The galaxy exhibits a disk-like morphology, although its presentation is more face-on than edge-on. There is evidence of spiral arm structure, and the arms appear somewhat flocculent rather than grand design. A central bulge is present, but it appears relatively small compared to the overall extent of the disk. The galaxy displays a blueish hue, suggestive of ongoing star formation. The overall appearance is somewhat disturbed. There is possible evidence of an interaction or merger with another galaxy. Patches of higher surface brightness are observed throughout the galaxy.
