The galaxy presents a relatively smooth and concentrated light profile, suggesting an elliptical morphology or a spiral galaxy viewed face-on with a dominant bulge. There are no obvious spiral arm structures visible.

The galaxy exhibits a yellowish-orange color, indicative of an older stellar population and lower star formation rate. This color suggests a population of evolved stars and a dearth of hot, young, blue stars.

There is a slight elongation in the shape of the galaxy. Some minor disturbances are visible in the immediate vicinity of the central body, which indicates possible recent or ongoing minor interactions.

Overall, this galaxy is likely a massive, relatively quiescent system with an old stellar population and signs of minor interactions.
