The galaxy presents a face-on spiral morphology. Two prominent spiral arms emanate from a central bar structure, displaying a grand design spiral pattern. The spiral arms exhibit loose winding, suggesting a relatively young stellar population and active star formation. There are hints of multiple dust lanes.

The bulge size is relatively small compared to the disk. There is a noticeable central brightening, indicating a possible active galactic nucleus or a dense concentration of stars in the nuclear region. A distinct color gradient is observed from the center outwards, with the core appearing yellowish-white, transitioning to bluish hues along the spiral arms, consistent with ongoing star formation. There is no evidence of any merging or major disturbances, implying a relatively isolated and dynamically stable system. The outer regions of the disk appear somewhat diffuse, suggesting a gradual decline in stellar density.
