The galaxy presents a distinct spiral morphology. It appears face-on, allowing for clear observation of its spiral arms. The arms are somewhat loosely wound and exhibit a clumpy structure, indicative of active star formation regions. These regions show bluer coloration, contrasting with the yellower hue of the central bulge.

The central bulge is relatively small compared to the overall disk size. There is no clear presence of a bar structure extending from the bulge.

The galaxy disk shows signs of possible disturbance, with some asymmetries in the spiral arm structure, suggesting minor gravitational interaction or past merger event. However, there is no other significant disruption visible.
