The galaxy presents as a spiral galaxy, observed at an oblique angle. The morphology suggests a disk-dominated system with tightly wound spiral arms. The light distribution across the galaxy is relatively smooth, with a central bulge. There is evidence of ongoing star formation activity, particularly within the spiral arms, indicated by subtle color variations across the galaxy. The galaxy appears to have a bar structure that extends from the bulge. There are no obvious signs of a recent major merger event; the system appears relatively undisturbed.