This galaxy exhibits a spiral morphology. The arms appear tightly wound, giving it a compact appearance. A central bulge is present, but it appears relatively small compared to the overall size of the galaxy. The disk is viewed at a near face-on orientation. The spiral arms are somewhat patchy, indicating varied star formation regions. The presence of multiple spiral arms suggests a grand design spiral structure. No significant signs of major merging or tidal disturbances are evident. A weak bar structure might be present in the central region. Overall, the galaxy appears as a relatively undisturbed spiral system with moderate star formation activity.
