The galaxy exhibits a spiral morphology, with a likely disk structure. The spiral arms are prominent, displaying a two-arm structure, although some areas are difficult to discern due to the image's resolution. The winding of the spiral arms is neither tightly wound nor loosely defined, appearing to be an intermediate pitch angle. A bar structure is present but subtle. The bulge of the galaxy appears to be moderate in size and brightness, less than the entire disk. There are several patches of blue star formation. The galaxy appears undisturbed. There are no indications of tidal tails or significant morphological distortions. Overall, the galaxy shows a well-defined spiral structure with ongoing star formation.
