The galaxy presents a generally smooth, elliptical morphology. There is a central bulge region appearing relatively bright and concentrated. Fainter regions extend outwards from the central bulge. The galaxy appears reddish-yellow in color, potentially indicating an older stellar population. There is a slight suggestion of disturbances or tidal features, which could be due to a potential minor interaction with another galaxy. However, based on its relatively smooth appearance, a prior merger is more probable. The light is concentrated towards the center and gradually diffuses outward. There is a possible, albeit subtle, disc structure. The overall impression is of a large, evolved system.
