The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth overall appearance. The core region exhibits a yellow-ish hue, suggesting a population of older stars. Moving outward from the center, the color transitions to a slightly bluer tint, possibly indicating the presence of younger stellar populations or regions of ongoing star formation, albeit at a low rate. There's no discernible spiral arm structure or prominent dust lanes. The galaxy appears relatively undisturbed, without signs of ongoing major mergers or tidal distortions. The shape is approximately round, displaying minimal elongation or asymmetry. The overall impression is that of a relatively evolved galaxy.
