The galaxy exhibits a distinct spiral morphology. Two prominent spiral arms emerge from a bright, relatively large central bulge. These arms are loosely wound and appear relatively open. The light distribution indicates ongoing star formation, traced by the bluer hues within the spiral arms. The bar structure in the central region of the galaxy appears fairly strong. Overall, the galaxy has a somewhat flattened appearance and may be viewed at a slight inclination. There are some minor disturbances potentially caused by a recent merger.
