The galaxy presents a distinct spiral morphology, exhibiting a prominent disk structure. The spiral arms appear well-defined and loosely wound, with a dominant two-arm structure that wraps around the central bulge. The bulge itself exhibits a moderate size relative to the disk. The galaxy displays a subtle bar-like structure extending through the bulge region, but is is not easily distinguishable. No significant signs of recent or ongoing merging events are apparent, but there may be some minor disturbance in the arms.
