The galaxy presents a morphology consistent with a late-type spiral galaxy. The structure exhibits prominent spiral arms that appear tightly wound and well-defined, indicating a grand design spiral structure. The arms are generally blue in color, suggesting active star formation regions populated with young, massive stars. Dust lanes are evident, especially along the inner edges of the spiral arms, contributing to the obscuration and reddening of light.

The central bulge of the galaxy appears relatively small and moderately bright, exhibiting a yellowish hue, likely indicating an older stellar population. The color gradient suggests a radial change in stellar population, with bluer colors dominating the outer regions.

Visually, the galaxy exhibits a disturbed morphology, with some asymmetry in the spiral arm structure, hinting at possible interactions or merger events in its past or ongoing tidal distortions. There is a pronounced central concentration of light but no obvious bar structure is visible within the resolution of this image. The overall appearance suggests a substantial disk component.
