The galaxy presents a largely featureless, smooth appearance. It exhibits a generally elliptical morphology with a moderate degree of roundness. There is a slight elongation, but the overall shape is closer to circular. Its luminosity profile appears concentrated towards the center. Based on the color indices, it is likely that the stellar population is dominated by older stars. The lack of distinct spiral arms or prominent dust lanes further suggests a relatively quiescent, passively evolving system. There is some subtle evidence suggesting minor gravitational disturbance, but no strong signs of an active galactic nucleus. The system's color and morphology combined is indicative of a evolved elliptical galaxy.
