This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated bright core that gradually fades outwards, with a more diffuse halo. The shape is mostly round, showing no obvious signs of strong spiral arm structures or significant distortions indicative of recent major mergers. There may be subtle hints of faint, extended features surrounding the main body, potentially tidal debris or a diffuse stellar halo, but it's difficult to confirm without higher resolution data. The color profile suggests a population dominated by older stars, with a relatively low rate of on-going star formation, consistent with typical elliptical galaxies. There are no visible dust lanes or prominent star-forming regions.
