The galaxy presents as a spiral type. It displays a distinct disk structure with evidence of prominent spiral arms. The arms appear tightly wound, suggesting a higher rate of shear. A central bulge is visible but it appears to be of moderate size, possibly encompassing about half of the galaxy's radius. A weak bar feature appears to be present within the central region of the galaxy. The disk component dominates over the bulge. The overall color of the galaxy is yellowish-red, indicating it is composed primarily of older stars. Signs of minor disturbances and potential merging activity are present with some disruption in the disk structure.
