The galaxy presents as a spiral type, with a clear disk structure viewed at a near-face-on angle. Two prominent spiral arms are visible, exhibiting a moderate winding. The central region appears to be dominated by a significant bulge component which presents itself as moderate in size. There is a bar feature across the galaxy, and it appears to be strong. Based on the image, it does not appear to be undergoing any major mergers, but some minor disturbances can not be ruled out. 
