The galaxy presents a centrally concentrated bulge, appearing smooth and yellow-orange in color, suggesting an older stellar population. Surrounding the central bulge is a fainter, disk-like structure, exhibiting a greenish-blue hue. This potentially indicates ongoing star formation within the disk. The disk appears somewhat disturbed, with faint asymmetries and possible tidal features, but the bulk of the galaxy appears without any major mergers. The overall morphology seems to be an intermediate spiral galaxy, with a prominent bulge and hints of a distorted disk.
