That is an interesting thought, Ames. I don't know a lot about the polar layered deposits, but I thought they were composed of layers of water ice, CO2 ice, and aeolian sediments. Your comment caused me to look up the density of CO2 ice, which is reported to range between ~ 1.3 and 1.6 gm/cm^3. So, water ice should be buoyant in CO2 ice.
We know that glaciers of water ice flow at earthly temperatures, but I would assume that flow is slower in current Martian temperatures. I don't know if CO2 ice can flow, but since it is held together by Van der Waals force, it probably can.
I hope some folks who know more about these layered polar deposits comment. There is a lot of thickening and thinning observed in the polar layers recently imaged by HiRise. Much of that appears to be due to depositional/erosional processes, but some of it resembles the density induced flows seen in buried salt layers on Earth, which flow more slowly than ice. I haven't found any
diapirs, but this concept is intriguing.