The galaxy presents a largely smooth, elliptical morphology. Its central region is characterized by a bright, concentrated light profile, exhibiting a yellowish-orange hue. The outer regions of the galaxy fade gradually into the background sky, displaying a more diffuse distribution of light. There is faint evidence of a very subtle disc, but it is very difficult to distinguish. The roundness of the galaxy is evident, with minimal deviation from a circular shape. There appears to be a general lack of significant tidal disturbances or prominent merging features, suggesting relative isolation and stability, although there are hints of some minor disturbances.
