The galaxy presents as a lenticular or early-type spiral, viewed at a moderate inclination. It exhibits a prominent, relatively smooth bulge component which appears generally spheroid. The disk is subtle, but visible, with a hint of bluer light suggesting some star formation. No distinct spiral arm structure is discernible. The galaxy is dominated by light at the red end of the spectrum. There are no signs of strong tidal features, major mergers, or significant dust lanes. There is slight light emission on the edges of the galaxy. Overall, the galaxy appears relatively undisturbed and evolved.
