The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge with a noticeable decrease in luminosity moving outwards. The overall color is yellowish-red, suggestive of an older stellar population with minimal ongoing star formation. There is no apparent disk structure or spiral arms. The shape is close to round. There are no indications of major mergers or tidal disturbances affecting its morphology. A faint, diffuse halo is possibly present but difficult to discern clearly.
