The galaxy appears to be a spiral galaxy, viewed at a significant angle. The galaxy shows prominent spiral arms, with a noticeable blue hue suggestive of ongoing star formation. The central bulge is not very prominent and may not exist at all. The disk appears relatively thin and has a disturbed morphology with some possible merging components. There is evidence of internal disturbances, with a noticeable asymmetry in the arm structures. There seems to be no strong central bar.
