The galaxy appears to be an elliptical type with a smooth, centrally concentrated bulge. There is evidence of a disk-like structure, but it is not well-defined and appears diffuse, showing very little spiral structure. Color gradients suggest an older stellar population, with redder colors dominating the central regions, and bluer colors present in the surrounding areas. There appears to be some minor tidal disturbance or ongoing merger activity visible. Overall, the galaxy's morphology suggests it is a relatively massive system.
