The galaxy presents an elliptical morphology, appearing largely smooth and featureless in this image. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards from the core. The galaxy possesses a yellowish-red hue, suggesting a population of older stars and a relatively low ongoing rate of star formation. There is no discernible spiral arm structure or dust lane present, reinforcing its classification as an elliptical galaxy. The galaxy appears relatively isolated, showing no strong signs of tidal interaction or recent merger activity, although a minor asymmetry cannot be completely ruled out. The overall impression is of a massive, quiescent galaxy with a significant stellar mass.