The galaxy presents a primarily smooth, elliptical morphology. It displays a concentrated central bulge that transitions into a less defined, more diffuse halo. There is no apparent spiral arm structure. Color gradients are present, with the central region appearing yellowish-white, suggesting an older stellar population. The outer regions show a subtle reddish tint, indicating a lower rate of star formation and the presence of cooler, older stars and dust. The galaxy exhibits a generally round shape, with only a slight deviation towards a more elongated form. No significant signs of tidal disturbances or ongoing mergers are visible.
