The galaxy presents a generally smooth, elliptical appearance with no readily discernible spiral arms or disk-like features. The morphology is characterized by a centrally concentrated bulge that dominates the overall light profile. The galaxy exhibits a gradual decline in surface brightness from the core outwards, with a diffuse halo extending into the surrounding space. It is an average size for galaxies, not particularly large or small.

There is evidence of minimal disturbance of the galaxy, though no mergers or strong tidal features are observed.
