The galaxy exhibits a clear spiral structure. The arms are well-defined and extend outwards from the central bulge, however it is difficult to resolve the exact number of arms present, though there are several. The winding of the arms appear moderately tight. The bulge appears relatively small and has a smooth appearance. The disk component is dominant. There is no apparent sign of a significant bar structure, though it is difficult to say with certainty. No major signs of galaxy interaction such as tidal tails or obvious distortions are observed, but there may be minor disturbances present. Overall, the galaxy appears as a relatively undisturbed spiral galaxy.
