The galaxy presents a distinct spiral morphology. Two prominent spiral arms extend from a moderately sized central bulge. The arms appear tightly wound around the bulge structure. The color of the bulge appears more yellow, suggesting an older stellar population. The spiral arms show a bluer tint, suggestive of active star formation. The overall structure appears relatively undisturbed, with no obvious signs of a major merger, although there might be minor distortions visible. There is a suggestion of a bar-like structure bisecting the central bulge.
