The galaxy appears to be a relatively smooth, elliptical system. It exhibits a bright, concentrated central bulge that gradually fades into a diffuse outer halo. There is minimal evidence of spiral arm structure or dust lanes. The color profile suggests a population of older stars, with a subtle bluer tint to the central region, potentially indicating some ongoing star formation or a younger stellar population in the core. The overall morphology is elongated, though nearly circular, suggesting a moderate degree of ellipticity. There are no obvious signs of tidal interactions or major mergers.