The galaxy presents a clear disk structure, exhibiting a well-defined spiral morphology. Predominantly, the spiral arms appear tightly wound around the central bulge. A moderate-sized bulge is visible, contributing significantly to the overall light profile of the galaxy. There is an indication of two prominent spiral arms. The disk is not perfectly face-on; there is a slight tilt. The galaxy exhibits a blue hue in its spiral arms, suggestive of ongoing star formation activity. There's no apparent major disturbance or significant signs of an ongoing merger.