The galaxy presents a spiral morphology with a relatively small and indistinct bulge. Its spiral arms exhibit a loosely wound structure, extending outwards from the central region. The arms appear somewhat flocculent and not sharply defined. Evidence suggests the presence of two prominent spiral arms. There are signs of interactions occuring within the galaxy, although whether they are due to a merger or minor disturbances within the disk is unclear. There is a faint bar-like structure appearing, however it is difficult to tell if it is a real bar, or part of the arm structure. Star formation is indicated by the blueish color of the galaxy, and possibly by the irregular morphology.