This galaxy presents a clear spiral structure, characterized by two prominent arms emanating from a central bar-shaped structure. The spiral arms exhibit a relatively tight winding pattern. The bulge component of the galaxy is moderately sized compared to the overall disk. Patches of intense star formation are apparent within the arms, indicating ongoing stellar birth. There is also evidence of minor gravitational disturbance within the galaxy, but it does not appear to be currently undergoing a major merger. The galaxy is not edge-on, and is viewed at an angle that shows the full spiral disk.
