The galaxy presents a prominent spiral morphology, with two distinct arms dominating its structure. These arms exhibit a loose winding pattern, extending outwards from the central bulge. The arms are not uniform in color, displaying both bluer regions indicative of ongoing star formation, and yellower regions that may indicate areas with older stellar populations or dust obscuration. The central bulge is relatively small, and does not appear to dominate the galaxy's overall light distribution. Evident is a disturbance to the lower right of the disk from a major merger. There is also a merging galaxy in the upper left. Overall, the spiral structure gives an appearance of being very pronounced despite a lack of uniformity. 
