The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with a high degree of roundness. The light profile suggests a bulge-dominated system with a smooth transition into the outer regions. There is no visible evidence of spiral arms or a distinct disk structure. The color gradient indicates a redder core region, potentially populated by older stellar populations, transitioning to slightly bluer hues in the outskirts, which might be indicative of some residual star formation activity, although the overall star formation rate is expected to be quite low. There is no strong evidence of tidal features or ongoing mergers, suggesting it is a relatively isolated system. Overall, it likely represents a massive and relatively quiescent galaxy.
