The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms appear loosely wound and possess a two-armed morphology. A bar structure seems to be present in the central region of the galaxy. The bulge is moderate in size relative to the disk. Star formation appears to be present across the galaxy, although there are no visible HII regions. The galaxy does not appear to be undergoing a major merger, though minor disturbances or interactions are possible. The axial ratio suggests that the galaxy is viewed at a moderate inclination.