The galaxy presents as an elliptical morphology, appearing largely smooth and rounded. It displays a color gradient, with a more yellow and centrally concentrated core. The outer regions exhibit a fainter, slightly bluer hue compared to the core, suggesting the presence of a younger stellar population in these areas, though the overall blue contribution is minimal. No significant disk features or spiral arms are discernible. There are no obvious signs of tidal disturbances or major mergers, although a slight asymmetry on one side might indicate a minor interaction or internal activity. Overall, the galaxy appears to be a relatively quiescent system.
