The galaxy presents a generally smooth, elliptical morphology. The light profile exhibits a concentrated core that gradually fades towards the outer regions. The color gradient suggests a population of older stars dominating the central region, indicated by the yellow-orange hue, while the outskirts show a slightly bluer tint, which could suggest more recent, albeit subdued, star formation activity. There are no visually apparent spiral arm structures or dust lanes. There is no apparent major disturbance or interaction with another galaxy, however there is a very subtle asymmetry which could imply minor disturbance. Overall, the galaxy appears to be a relatively quiescent system, possibly undergoing slow evolution.
