The galaxy appears to be a spiral galaxy viewed at a significant inclination. There is a prominent central bulge that is elongated along the major axis of the disk, with some mottling and possible dust lanes visible within the bulge. The disk appears to be relatively smooth, but with an indication of spiral arms, potentially two or three, that are tightly wound. The color suggests that it is forming stars at a modest rate. The overall structure is somewhat disturbed, as evidenced by the faint and irregular outer regions, which could be indicative of a minor interaction or a recent merger event. The galaxy is roughly 4.5 kpc across in its widest dimension.
