The galaxy appears to be a spiral galaxy, observed at an angle between face-on and edge-on. There appears to be a relatively bright and prominent central bulge. The spiral arms are not well-defined, appearing somewhat flocculent, with regions of blue light indicative of active star formation scattered throughout the disk. There is a hint of dust lanes in the disk, particularly visible on one side of the bulge. The galaxy exhibits a degree of internal structure, suggesting possible minor disturbances.
