This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, surrounded by a more diffuse halo of light. The galaxy appears to have a fairly uniform color profile, lacking prominent spiral arm structures or distinct dust lanes, which suggests a relatively old stellar population with little ongoing star formation. It has an intermediate shape between round and elliptical. There does not appear to be any strong evidence of any mergers or tidal interactions, but a small portion of the sample indicates there might be a slight disturbance. 
