The galaxy presents as a relatively smooth, disk-like structure with an apparent elliptical morphology from our viewing angle. Its color profile suggests a population of older stars, appearing more yellow and red. The galaxy's shape is somewhat elongated, with a cigar-like appearance rather than a perfect circle. There is a hint of a central bulge where the light is concentrated. The disk appears to be relatively undisturbed, with no obvious signs of a major merger or significant tidal disruption. Some minor disturbances or irregularities might be present within the disk structure.