The galaxy presents a spiral morphology with a clear central bulge. The spiral arms appear tightly wound around the central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population, while the arms show a bluer tint, which could indicate ongoing star formation. There are multiple spiral arms with several strands of dust and gas. The overall form suggests the galaxy is relatively undisturbed. There are no signs of extreme tidal disruption or major merging activity. The light appears generally well distributed.
