The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears moderately diffuse, lacking strong spiral arm structures or a prominent bulge component. There's a slight elongation evident, deviating marginally from a perfectly circular shape, but it is mostly round or in between. The color profile suggests a population of older stars, with a tendency towards redder hues overall, though it does show a range of color. There are no immediately obvious signs of ongoing major mergers or tidal interactions, though some minor disturbances cannot be ruled out. There may be some presence of a disk. The galaxy exhibits a relatively modest apparent angular size.
