This galaxy presents as a flattened, elongated structure, suggesting it is likely a spiral galaxy viewed at a high inclination. Its central bulge appears to be a concentrated region of older stars, exhibiting a yellow-red hue, while the surrounding disk is a lighter blue color, suggesting recent star formation. The galaxy appears to have a smooth texture with the hint of spiral structure in the disk. The relative color and light intensity suggests a considerable mass and ongoing star formation processes. There is no obvious presence of any ongoing major mergers or disturbances, though minor disturbances in the disk cannot be ruled out.