The galaxy presents a largely smooth, elliptical morphology. Its light is concentrated towards the center, with a gradual decrease in surface brightness moving outwards. The core region exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions appear bluer, suggesting some ongoing, although subdued, star formation activity. There is no obvious presence of spiral arms or a distinct disk structure. The object appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. Faint asymmetric features might be present in the outer regions, possibly indicating minor disturbances. The galaxy has a generally round shape, with only a slight deviation towards an elongated form.
