The galaxy presents as a spiral galaxy, with a prominent disk component. The spiral arms are tightly wound, appearing in a grand design structure originating from a central bulge. The bulge contributes substantially to the galaxy's overall luminosity. A bar structure is present across the central bulge, contributing to the spiral arm morphology. The dust lanes within the spiral arms are well-defined, indicating ongoing star formation, but at a low rate. The galaxy shows no obvious signs of recent major mergers, but there is a small indication of a minor disturbance. The morphology is likely that of a fairly massive galaxy.