The galaxy presents a flattened, disk-like morphology, oriented approximately horizontally in the image. It appears to exhibit a central, brighter region, suggesting a galactic bulge or core. The disk appears to have some structure, though not sharply defined spiral arms. There is a subtle color gradient visible across the disk, with a bluer hue possibly indicating regions of younger stars and star formation. The outer regions of the disk are less defined and more diffuse. There may be minor disturbances indicating potential tidal interactions or minor mergers.