The galaxy presents as a lenticular or early-type spiral galaxy, appearing largely smooth with a dominant bulge component. The central bulge exhibits a yellowish-white hue, suggestive of an older stellar population. The disk, while not sharply defined, shows a slight flattening and appears bluer in color, possibly indicating the presence of younger stars and ongoing star formation. There appears to be some subtle, diffuse structure within the disk, but no distinct spiral arms are readily apparent. The overall shape is somewhat elongated, deviating slightly from a perfect circle. There is no obvious evidence of tidal interactions or major mergers. Subtle irregularities might suggest minor disturbances in the recent past.
