The galaxy presents as a smooth, centrally concentrated elliptical type. Its morphology is generally rounded. There is no obvious disk structure. The light distribution indicates a fairly homogenous stellar population, lacking prominent features. There is a central bulge evident. A subtle color gradient suggests older stellar populations are centrally concentrated, with perhaps slightly younger, bluer stars extending outwards. There is no evidence of recent or ongoing major merger activity, though minor disturbances are not ruled out. Overall the galaxy appears relaxed and relatively undisturbed.
