The galaxy presents as a relatively smooth, centrally concentrated object. There is a noticeable color gradient, with the central region appearing more yellow-white, suggesting a population of older stars. The outer regions appear slightly bluer, hinting at the presence of some younger stars, though not in significant quantities. The overall morphology appears elliptical to slightly disk-like, but with a high degree of central concentration. There is no obvious indication of spiral arm structure. Subtle irregularities and disturbances indicate possible minor interactions or a past merger event, but the galaxy appears mostly relaxed, without strong tidal features. The overall color suggests it is likely a galaxy with moderate star formation, but it is primarily composed of older stars.
