The galaxy exhibits a spiral morphology, presenting with well-defined, prominent spiral arms. These arms emanate from a central bulge region. A distinct winding pattern in the spiral arms can be observed with most appearing moderately tightly wound. The galaxy appears face-on. The bulge appears relatively small compared to the overall disk size. The color distribution indicates a higher concentration of older stellar populations in the central bulge, transitioning to bluer, star-forming regions within the spiral arms. There is some evidence of irregular features or distortions, possibly indicating minor gravitational interaction or internal disturbances. Dark dust lanes are apparent within the spiral arms. Star formation is occurring within the arms.