The galaxy presents as a centrally concentrated, elliptical-like structure. Its core appears bright and smooth. Fainter light extends from the center, creating a diffuse halo. The shape is more elongated than circular, but not exceptionally so. There is no obvious dust lane or spiral arm structure discernible. There is no strong visual evidence of a major merger event, though a minor disturbance cannot be ruled out. Overall, the galaxy appears as a relatively evolved system.
