The galaxy appears to be a relatively smooth, elliptical-like system, exhibiting a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. It shows a lack of prominent spiral arm structures or distinct dust lanes. The overall color is slightly reddish, suggesting a population dominated by older stars and a low rate of ongoing star formation. There may be some minor gravitational interaction occurring as there appears to be some minor disturbances, with possible tidal features in the out regions, though no obvious signs of a major merger are detected. The galaxy seems to have a high degree of rotational symmetry, appearing nearly round in shape.
