The galaxy presents a disk-like structure with prominent spiral arms. The arms appear tightly wound in some regions and more open in others. The morphology suggests a grand design spiral structure. The galaxy exhibits a notable central bulge, though not excessively dominant. The color gradient indicates a relatively actively star-forming galaxy, showing bluer regions in the spiral arms where star formation is more prominent, and yellower color in the central bulge. A weak bar may be present, but it is not highly distinct. There is no apparent evidence of a major merger, but some minor disturbances may be present.
