The galaxy presents as a flattened, elongated structure with a distinct cigar-like morphology. A central bulge, appearing yellowish, dominates the core region and gradually fades into a disk. The disk exhibits a bluer hue, particularly at one end, suggesting the presence of younger, hotter stellar populations, and potentially ongoing star formation regions. The opposite end is less distinctly blue. There are possible minor disturbances present in the disk of the galaxy, although they are not drastically disrupting the overall structure. Overall, the galaxy appears relatively smooth.
