The galaxy presents a defined spiral structure with two prominent arms. These spiral arms appear somewhat tightly wound. A bar structure is possibly present, bisecting the central bulge, though its strength is difficult to ascertain from this image. The central bulge is a significant fraction of the galaxy's overall size. The overall color suggests a mature stellar population, though bluer regions imply ongoing star formation. There is no evidence of a major merger. Some evidence points toward minor disturbances in the disk. The galaxy is not viewed edge-on.
