This galaxy exhibits a prominent spiral structure. Two spiral arms are distinctly visible, appearing loosely wound. A moderate-sized bulge is present at the galaxy's center. The overall structure suggests that this galaxy is undergoing a merging process. The merging process is likely a major disturbance to its structure, though it doesn't appear overly deformed. The presence of spiral arms suggests ongoing star formation within the disk. The galaxy displays a relatively normal disk structure when not taking the merging into account. A bar shape is neither especially strong or weak. 
