The observed galaxy presents a clear spiral structure, though somewhat indistinct. The spiral arms appear to be relatively tightly wound around the galactic center, indicative of a grand-design spiral. The galaxy exhibits a moderate bulge component, but the disk appears to be the dominant feature. There is no clear indication of a strong central bar structure. The galaxy is observed face-on, or nearly so. Some disturbances in the disk are present, but it is not obviously undergoing a major merger. Star formation appears to be present, but it is not a particularly high amount.
