The galaxy exhibits a prominent disk structure with a clearly defined spiral pattern. The spiral arms appear grand design, demonstrating a sweeping, well-defined morphology. The winding of these arms appears to be of medium pitch, suggesting a balance between tightly wound and loosely dispersed structures. It appears to be a barred spiral galaxy with a noticeable bar structure in the center. The bar exhibits a substantial presence across the galaxy's central region. The presence of a bulge is evident, though it appears to be relatively small and less luminous, suggesting a lower concentration of stars compared to the disk. In addition, the light and colors suggest it is experiencing ongoing star formation. There is no evidence of a major ongoing merger event, and the overall structure shows a relatively undisturbed morphology.
