Just look at the sky at night. Almost all the stars that are visible in the night sky are at least as large as the Sun. From a strict angular subtense perspective, they are almost all smaller in width than a 2ft tower at 5 miles. The sun, if moved to Alpha Centauri's location, would subtend about 7 milli-arcseconds. Now, of course, the atmosphere diffraction limit is about 2 arcseconds, so the objects aren't as small as they should be. But, that's still smaller than the 5 arcseconds that the tower would subtend.
Nonetheless, you can "see" them, i.e., tell the difference between them and their background, which was the question I posed about what is meant by "see." So, if the tower was adequately contrasted with its background, you could "see" it. There would be no detail, nor any indication of actual width, but again, that's not necessarily required to achieve "seeing"
Note that this is fundamentally different that "resolving" 2ft at 15 mi. That would require you to tell the difference between 2ft objects spaced 2ft apart at 15 mi, which is impossible with the naked eye.
As we know, detailed understanding of the requirements spells the difference between success and failure, so the OP needs to define his problem more precisely.
TTFN
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