The galaxy presents as a smooth, centrally concentrated object. It appears to be fairly elliptical in shape, though not perfectly so. The color is yellowish-white, indicating a population of older stars with likely little ongoing star formation. There is a subtle suggestion of a disk-like structure, but overall it seems to be mostly bulge dominated. There is no clear evidence of tidal tails, major mergers, or significant dust lanes. Some minor asymmetry might be present, but more data is needed to characterize this. The galaxy appears relatively isolated and undisturbed.
