The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, trending toward a round shape. There is some indication of minor disturbance or merging activity, possibly indicated by slight asymmetries or irregularities in its overall structure. The galaxy has a prominent central bulge or core with a diffuse halo. The galaxy has a redder hue than other objects nearby, implying an older stellar population and reduced star formation.
