The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure with prominent spiral arms. The arms are loosely wound and have a moderate amount of fragmentation. There is a noticeable central bulge; It is rather small and unassuming, with the disk dominating the overall appearance of the galaxy. There appears to be a relatively high level of ongoing star formation, inferred from the blue color of the spiral arms. The galaxy also possibly has a weak bar structure. The image shows no definitive signs of a major ongoing merger event; however, there appears to be a minor visual disturbance.
