The galaxy presents a moderately elliptical morphology, appearing largely spheroidal with a slight elongation. Its light profile indicates a concentration of luminosity towards the core region, which exhibits a yellowish-white hue. The color gradient suggests an aging stellar population dominating the central region, characteristic of older stars. Extending outwards from the core, a bluer diffuse halo is observed, hinting at a possible presence of a younger, though less prominent, stellar population contributing to star formation activity. The overall structure exhibits a relatively smooth appearance, suggesting a lack of major disturbances or ongoing mergers. There's a subtle asymmetry in the outer regions, potentially indicating minor interactions or past tidal effects.
