The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, diffuse luminosity profile, with the intensity decreasing gradually from the core outwards. There is no evidence of spiral arms or a distinct disk component. The galaxy's color appears to be moderately red, suggesting an older stellar population, but is a bit more colorful closer to the center. There is no obvious evidence of ongoing major mergers or strong tidal disturbances from this image. The overall form suggests it is likely a galaxy that has undergone significant dynamical relaxation.
