The galaxy appears as a moderately luminous, elliptical-shaped object with a smooth, centralized light distribution. The color profile indicates a generally older stellar population. The light in the center has a subtle green tint. The galaxy appears mostly undisturbed, displaying no obvious signs of recent major mergers or strong tidal interactions. Given its apparently high degree of smoothness and lack of spiral arm structures, the galaxy is likely an elliptical galaxy. The lack of noticeable dust lanes or prominent HII regions further support this classification. Overall, the galaxy appears to be a relatively evolved system, likely with a low specific star formation rate.
