There has been tremendous progress on DUNE over the past few years, driven by a very dedicated collaboration. Over the next few years, DUNE will be going through at least two important transitions. The first will be triggered by decisions made in the US ``P5'' process. While the US SNOWMASS process recommends the most important directions for the next several years, P5 sets priorities---and therefore, funding and schedules---for all of the US HEP. We must ensure that we make a convincing case that our full Phase II physics program, including additional detector mass, upgraded beam, and near detector suite, is a compelling high-priority program that must move forward as quickly as possible. Success here will require us to reiterate our precision capabilities for DUNE's primary physics, and also point out that the once-in-lifetime investment in neutrino physics that has already begun can leverage an even broader scope of science---turning LBNF/DUNE into a world-leading place to explore the rich array of physics available in our field. The second transition will happen if we maintain, and hopefully advance, our current Phase I schedule. Just think: graduate students recruited in the next two or three years will actually see neutrino data from DUNE itself. We will thus start changing from a project, to an experiment. We must go beyond our sensitivity studies and tool development and begin thinking how we will RUN the DUNE experiment, and how we will extract physics. We will need to take lessons learned from ProtoDUNE analyses---and those of the short-baseline program---to ensure we will be ready on Day 0 to start producing precision physics. And we need to do all of this while insisting that our collaboration move forward on our shared goal of diversity along all the axes on which we have done poorly historically. We should explore ways in which we can better involve minority-serving institutions in our work, for example, by involving students even now when we are heavy with project engineering. We also need to strengthen the inclusivity of our collaboration by always being clear that the DUNE Collaboration conducts itself with mutual respect for everyone. Priorities over the next few years are therefore: o Ensure we maintain or advance the Phase I schedule. Doing this may require creativity, and it may require hard choices, but as DUNE data peeks above the horizon, it will catalyze a resurgence of scientific effort from across the collaboration. o Succeed in convincing P5 that all of Phase II is critical to our program and to the field as a whole, and that it must move forward as quickly as possible. We should include an argument that a broad program is possible at LBNF/DUNE, and that goal will inform our choices of technology for Modules 3 and 4. o Broaden participation in DUNE, particularly from under-represented and marginalized groups, and ensure that we maintain a respectful environment for everyone. o Take the lessons learned from ProtoDUNE and other LArTPC data analyses, to streamline our own approaches. We need to be ready with a plan for getting physics from DUNE on timescales much shorter than what our community has done to date.