The galaxy appears to be a relatively smooth, lenticular or early-type spiral. The central bulge exhibits a concentrated, bright yellowish-white hue, indicative of an older stellar population. Fainter bluish light extending out from the central region suggests the presence of younger stars and possibly some star formation, though this feature is not dominant. The overall shape of the galaxy is somewhat elliptical and moderately round, showing no strong indication of significant tidal disturbances or ongoing major mergers. Some minor disturbances cannot be ruled out, however, based on the morphology.
