This galaxy presents a primarily smooth, elliptical morphology. The light profile exhibits a centrally concentrated bulge with a gradual decrease in luminosity outwards. While there is some indication of a disk component, it is not well-defined, suggesting a relatively low level of organized rotation. There is no evidence of strong spiral arm structures or significant dust lanes within the galaxy. The central region displays a yellowish hue, indicative of an older stellar population. There are faint bluish tinges in the outer regions which hint at a small amount of recent star formation. The overall structure suggests that the galaxy is likely a mature system. No major disturbances or signs of mergers are observed.
