The galaxy exhibits a disk-like structure, though the exact inclination angle is difficult to discern. There is evidence of spiral arms present, indicated by subtle color and luminosity variations within the disk. The central bulge is moderately sized, though it does not dominate the overall appearance of the galaxy. The morphology suggests it is in the process of undergoing a merger, or has recently experienced a merger event; there is clear morphological disturbance. It has a moderate amount of star formation. 
