The galaxy presents a disk-like structure with a central bulge. The morphology indicates a spiral galaxy, viewed at a moderate angle, not edge-on. Spiral arms are clearly visible, displaying a multi-armed structure, approximately three distinct arms. The arms appear moderately wound, neither tightly nor loosely coiled around the nucleus. There is evidence of a bar-like structure spanning through the central region of the galaxy, although it is not highly pronounced. The bulge appears moderate in size. The galaxy does not display signs of major merging activity. However, a minor disturbance may be visible, potentially due to a past interaction or ongoing accretion. There appears to be active star formation within the galaxy.
