The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions of the galaxy appear fainter with a subtle reddish tone, possibly indicating a lower density of stars or the presence of dust. There is no obvious evidence of spiral arms or active star formation regions visible. The overall morphology implies a passively evolving galaxy, likely an elliptical or lenticular type, with a smooth, round shape. No signs of tidal disturbances or major mergers are apparent.
