The galaxy exhibits a disk-like morphology, oriented at a slight angle relative to the observer's line of sight. Prominent spiral arms are visible, tightly wound around a central bulge. The bulge appears relatively small compared to the overall size of the galaxy. The spiral arms show a two-armed structure, though some arms may be more complex, hinting at branching. The arms present a smooth texture, without signs of clumpy star formation regions. The galaxy appears undisturbed, without major signs of ongoing mergers. There may be a slight asymmetry of the spiral arms, suggesting possible minor interaction in the past. A faint bar structure may be present in the central region, though not prominently defined. The dust lanes are visible within the arms.
