The galaxy presents as a relatively smooth, elongated structure, suggestive of a disk galaxy viewed edge-on. There is a slight concentration of light toward the central region, possibly indicating a bulge, though it is not distinctly pronounced. The color is primarily bluish, with a slight reddening visible near the edges of the disk. This blue hue suggests the presence of a younger stellar population and ongoing star formation. There does not appear to be evidence of strong spiral arm structure or significant dust lanes. There is a hint of minor disturbances, but overall, the galaxy's morphology appears largely undisturbed, showing no obvious signs of a major merger. The galaxy is moderately luminous, and its compact appearance indicates a high stellar density.
