The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated central bulge with a gradual decrease in luminosity towards its outer regions. It is characterized by a moderate ellipticity, appearing somewhat flattened along its minor axis. The light profile suggests a relatively high Sersic index, indicative of a centrally concentrated light distribution. The color of the galaxy appears to be predominantly yellow/white, suggestive of a stellar population dominated by older, redder stars. There is no obvious evidence of distinct spiral arms or significant dust lanes. The galaxy does not seem to show any signs of recent major mergers or strong tidal disturbances. The overall structure appears relatively undisturbed and well-defined.
