The galaxy appears to be a relatively smooth, centrally concentrated system, likely an elliptical or lenticular type. It exhibits a dominant, round bulge with a yellowish-white color, suggestive of an older stellar population. There is some indication of an extended, fainter halo surrounding the central region, with a slight elongation. The color gradient appears to be relatively uniform, though subtle variations might indicate underlying structure. Faint blue-ish hints may signify a small amount of ongoing star formation, although the overall color suggests it is quiescent. There are no obvious signs of spiral arms or a prominent disk. The galaxy does not appear to be undergoing any major merging or interaction with other galaxies.
