The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge which graduates into a less luminous, more diffuse halo. The overall color appears to be yellowish-orange, suggesting a population of older stars with relatively low ongoing star formation. The galaxy lacks any obvious spiral arm structure or prominent dust lanes, although the central bulge may contain some unresolved features. There are no indications of major mergers or significant tidal disturbances. The overall appearance suggests a galaxy nearing the end of its star-forming life.
