The galaxy presents as a lenticular or early-type spiral with a prominent central bulge. The bulge exhibits a relatively smooth light distribution. Faint, diffuse features can be seen, which may constitute a weak disk component. The overall shape is close to circular, though there's a slight elongation observed. No strong evidence of a recent major merger or tidal disturbances are observed, although some subtle asymmetry may suggest past minor interactions. The galaxy appears yellowish-red, suggesting an older stellar population.
