The galaxy presents a distinct spiral morphology. The arms are tightly wound and are fairly well-defined. There appears to be multiple arms that are quite well-defined, giving the galaxy a structured appearance. The central bulge is of a moderate size in comparison to the overall disk. Star formation appears to be active within the spiral arms, as suggested by the blue-ish hue. No obvious signs of a major merger are visible, but a slight disturbance can not be ruled out. There may be a weak bar structure present in the central region. The galaxy is not edge-on, instead it is at a fairly low inclination angle.
