The galaxy exhibits a distinct spiral structure. The arms appear relatively tightly wound around a central bulge. The bulge constitutes a moderate portion of the galaxy's overall size. Three major spiral arms can be discerned emanating from the central bulge. These arms show subtle color variations, suggesting ongoing star formation. The overall disk orientation is face-on. A weak bar structure is visible extending across the central region. There is no apparent evidence of a major merger event affecting the galaxy's morphology, though minor disturbances cannot be ruled out. The galaxy is mainly blue, representing younger, more active stars.