The galaxy presents as a spiral type. Its overall color suggests a mix of stellar populations. The central bulge appears relatively small and bright, indicating a concentration of older stars. Spiral arms are clearly visible, although somewhat tightly wound. There may be signs of multiple arms. The spiral arms appear slightly patchy, hinting at regions of ongoing star formation. The disk appears face-on, as indicated by its circular shape. Overall, the galaxy seems relatively undisturbed, lacking significant signs of major merger activity. The galaxy exhibits no distinct bar structure.
