The observed galaxy presents as a flattened, disk-like structure viewed edge-on. A bright, central bulge is not clearly apparent. The dominant feature is a bright, relatively thin disk exhibiting distinct color variations. The inner regions of the disk display a vibrant blue hue, transitioning to a green, then yellow, tint further away from the center. These color gradients suggest ongoing star formation within the disk, with younger, hotter stars concentrated in the inner regions and older, cooler populations located at greater distances.

The galaxy also appears to exhibit signs of tidal interactions or minor disturbances. A slight warp in the disk's structure and faint extended emission surrounding the galaxy hint at these phenomena. While a major merger is not apparent, the overall morphology suggests a system that has experienced past interactions with other galaxies or is currently undergoing minor accretion events.
