The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, displaying a high degree of roundness in its overall shape. There is a distinct lack of discernible spiral arm structure or prominent dust lanes. The light profile suggests a centrally dominant bulge, with a gradual decrease in luminosity moving outwards. Color gradients indicate a redder core region, potentially signifying an older stellar population with reduced ongoing star formation. The outer regions exhibit bluer hues, though this could also be a result of image noise. No significant signs of tidal disturbances or ongoing mergers are visible. The galaxy appears to be an evolved system with a substantial stellar mass and a low star formation rate.
