The galaxy exhibits a prominent spiral structure. The spiral arms appear well-defined and numerous, with a tightly wound morphology, particularly near the central bulge. The central bulge is bright and concentrated, suggesting a significant population of older stars. The overall color of the galaxy is skewed toward bluer hues, indicative of active star formation, particularly within the spiral arms. Some areas of the galaxy are diffuse and irregular, possibly due to minor gravitational interactions or recent starburst events. The disk is viewed at a moderate inclination, allowing clear observation of the spiral arm structure. There is no indication of a strong bar feature.
