The galaxy presents as a disk galaxy, viewed at a nearly edge-on perspective. It exhibits a bright, concentrated central bulge, appearing yellowish-white. There is evidence of a dust lane that is slightly obscuring the bulge. Extending outwards from the bulge are fainter regions that create a disclike structure. The disk appears to be slightly warped. There are knotty areas of the disk that appear to be areas of star formation. The overall color appears to be a slightly warmer hue than a typical spiral galaxy, indicating an older stellar population. There may be signs of interaction with a nearby galaxy.
