The galaxy appears as a relatively smooth, elliptical object, with no distinct spiral arm structures visible. Its color is somewhat red-shifted, suggesting an older stellar population and a relatively quiescent star formation rate. The galaxy's light is centrally concentrated, with a gradual decrease in intensity towards its outer regions. It exhibits a slight elongation, deviating somewhat from a perfectly circular shape. There is no strong evidence of any major disturbances or ongoing mergers. The galaxy exhibits a high Sersic index, indicating a centrally concentrated light profile, consistent with the observed smooth appearance. Overall, this appears to be a mature elliptical galaxy.
