The galaxy presents as a spiral type, exhibiting a disk structure viewed at a slight inclination. The morphology is characterized by prominent spiral arms, appearing somewhat flocculent, displaying multiple arms. The spiral arms are not tightly wound, with a moderate pitch angle. The central bulge appears to be of moderate size, with some evidence suggesting the presence of a weak bar structure. Star formation seems to be active within the spiral arms, indicated by the patchy blue hues distributed across the disk, with the inner disk appearing yellower. There may be a merger or minor disturbance.
