The galaxy presents as a centrally concentrated, primarily smooth system. It exhibits a roughly elliptical morphology. The core region appears bright and relatively homogenous, with a moderate degree of radial concentration in luminosity. The galaxy shows evidence of a weak, diffuse disk component. The disk appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Overall, the galaxy appears to be a relatively evolved system, undergoing moderate star formation. There is no evidence of significant dust lanes. The light appears to be dominated by older stellar populations.
