The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that graduates into a less luminous, more diffuse halo. Color gradients are subtle; the core appears slightly more yellow, potentially indicating an older stellar population, while the outer regions exhibit a bluer tint suggestive of some ongoing or recent star formation. There are faint disturbances present, but there is no definite sign of spiral arms or a prominent disk structure. The overall impression is of a galaxy that has largely completed its major mergers and is now in a relatively quiescent state, but there is evidence of minor interactions with other objects.
