The galaxy presents a largely smooth, elliptical morphology. The light profile appears concentrated, with a bright central core that gradually diffuses outward. The core exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the core is a more diffuse halo, displaying a faint bluish tinge, potentially indicative of some ongoing, albeit low, star formation activity. There is no apparent disk structure or spiral arm morphology. Evidence of tidal disturbances or merging activity is absent from the visible structure. The galaxy appears relatively isolated and undisturbed.
