The galaxy presents a flattened, disk-like morphology with a prominent central bulge. Faint spiral arm structures appear to emanate from the bulge, winding loosely. The color distribution indicates a relatively evolved stellar population in the bulge, appearing yellowish-white. The spiral arms exhibit bluer hues, suggesting ongoing star formation, though the resolution limits a detailed assessment of star-forming regions. The galaxy does not appear to be strongly barred. The overall light distribution suggests a smooth transition from the bulge to the disk, with no obvious signs of recent major mergers or tidal disturbances, though some minor disturbances cannot be ruled out based on the available imagery.
