The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. It is nearly round in shape, showing little to no discernible disk structure or spiral arms. The color gradient suggests a stellar population dominated by older stars, with a reddish hue dominating the core region. Fainter, more diffuse light extends outwards from the central region, gradually fading into the background sky. There's no obvious indication of ongoing major mergers or strong tidal disturbances, however, there may be minor asymmetries in the outer regions, possibly indicating past or ongoing interactions. The overall morphology indicates a well-evolved system, possibly a result of hierarchical merging and subsequent relaxation. It is a relatively low mass galaxy with little star formation occurring at this point.
