The galaxy presents a primarily smooth morphology. It exhibits a somewhat elliptical shape, with a bright, concentrated central bulge. The outer regions appear diffuse and less structured, displaying a gradual decrease in luminosity from the core to the edges. There is a subtle disk-like component. Overall the light seems to come predominantly from older stellar populations, as indicated by the yellowish hue in the central region. The galaxy does not show any obvious signs of strong tidal interactions or major mergers, and the disk may have some minor disturbances.
