The galaxy presents as a spiral type, exhibiting a moderately sized bulge that is neither dominant nor insignificant. A bar structure bisects the bulge, appearing to transition from strong to weak along its length. Predominantly, spiral arms emanate from the central region, and are tightly wound, almost flocculent in nature.

There is a slight amount of irregular structure within the arms and their pitch angle is small. The disk is not edge-on, appearing closer to face-on. The spiral arms are somewhat difficult to distinguish due to the tight winding and lack of high resolution.

The overall light distribution suggests this galaxy is undergoing moderate star formation. No major mergers are evident, though subtle asymmetries hint at possible minor gravitational interactions.
