The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated bulge that appears yellow, suggesting an older stellar population dominating the core. There may be an extended, fainter disk-like component surrounding the bulge, showing a bluish tint to the outer regions. These colors indicate the presence of younger, hotter stars, with hints of ongoing star formation. It is a fairly massive galaxy, appearing roughly circular. There appear to be no signs of tidal tails or major disturbances, which indicates no ongoing or recent major mergers. There is the potential for minor disturbance in the shape of the surrounding disk which hints at the possibility of interactions. Overall, the galaxy is likely a relatively evolved system.
