The galaxy exhibits a disk-like structure with noticeable spiral arm features. The arms appear somewhat patchy and loosely wound. A prominent central bulge is observed, less significant than the disk. Overall, the morphology suggests a spiral galaxy. There is a possible minor disturbance present in the galaxy's form, but the image's resolution does not provide clear evidence of a major ongoing merger. The galaxy's overall color appears relatively blue, potentially indicating active star formation regions within the spiral arms.
