The galaxy presents as a disk galaxy, viewed at a slight inclination. There is evidence of spiral arm structure, although somewhat flocculent. A central bulge is present, with an intermediate size relative to the disk. There may be a faint, subtle bar structure. Overall, the galaxy appears relatively undisturbed, without obvious signs of major mergers, although minor disturbances cannot be ruled out. The galaxy exhibits a blue hue, indicating ongoing star formation. The estimated size of the galaxy is a few kiloparsecs across.
