This galaxy exhibits a distinct spiral morphology, although somewhat flocculent in nature. The spiral arms are not tightly wound, appearing relatively open. Star formation is evident within the arms, highlighted by patches of blue light indicative of young, hot stars. A central bulge is present, but appears relatively small and not highly concentrated. There appears to be some minor interaction with nearby galaxies. There also appears to be some minor disturbance going on within the arms of this galaxy. There is a prominent bar structure that runs through the middle of the galaxy. Overall, the galaxy appears to have a somewhat irregular structure, with more light on one side than the other.
