The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated brightness profile with a gradual decrease in luminosity towards its outer regions. The overall color is slightly reddish, suggestive of an older stellar population and reduced star formation activity. There may be a faint disk structure present, but it is not a prominent feature. No major disturbances or signs of merging are readily apparent; instead, the galaxy shows a well-defined, singular structure with a high degree of circularity.
