The galaxy presents as a relatively smooth, elongated structure, consistent with a likely edge-on or highly inclined spiral galaxy. A central bulge is faintly discernible, appearing slightly brighter and more concentrated than the surrounding disk. The disk exhibits a general blueish hue, suggesting the presence of younger, hotter stars and ongoing star formation. Its apparent color becomes redder towards the center. Dust lanes are not clearly resolved in this image but cannot be ruled out. Based on its apparent size and morphology, the galaxy is likely of significant mass. The structure shows no strong evidence of major mergers or significant tidal disturbances, though minor disturbances or past interactions cannot be excluded.
