The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge, suggesting a high stellar density in the core region. The overall shape appears close to circular, showing little evidence of strong disk features. The color gradient indicates a population of older stars with a significant red component, particularly concentrated towards the center. There are hints of some bluer regions throughout the galaxy, which could be associated with younger stars. The galaxy does not exhibit any obvious signs of major mergers or tidal disturbances, although some faint asymmetric features could indicate minor interactions or internal structures.