The galaxy presents as a spiral type, with a prominent central bulge and a disk exhibiting spiral arm structure. The arms appear tightly wound around the central bulge. The galaxy's color indices suggest active star formation. The image indicates moderate-sized spiral arms. The galaxy does not appear to be undergoing a major merger, though there might be some minor disturbances in the morphology, indicating past interaction. The galaxy is observed nearly face-on. The spiral arms are tightly wound.
