The galaxy presents as a spiral type, with a disk-dominated morphology. Two prominent spiral arms are wound relatively tightly around the central bulge. The disk exhibits a moderate degree of patchiness, suggesting regions of active star formation within the spiral arms. The central bulge appears relatively small and not especially luminous compared to the disk. There is no obvious bar structure visible. The galaxy displays a blue hue within the spiral arms, indicative of younger stellar populations, while the bulge appears more yellowish, possibly indicating an older population of stars. There is no apparent interaction or major disturbance evident in its overall structure, though minor irregularities or distortions might be present upon closer inspection.
