The galaxy presents an elliptical morphology, appearing largely featureless and smooth in texture. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core gradually fading into the surrounding halo. The overall shape is somewhat elongated. The core has the appearance of older stars, while the outer regions appear to contain slightly younger stars. There is no obvious spiral structure or prominent dust lanes visible. There is no signs of a major merger. There may be a minor disturbance occurring.
