The galaxy appears to be a flattened, disk-shaped system, observed nearly edge-on. It exhibits a central bulge that appears relatively smooth and amorphous, transitioning into a fainter disk. Within the disk, there is a slight hint of substructure. Light from the galaxy displays a range of colors, with a slightly bluer hue dominating the disk. This implies ongoing star formation activity. The outer regions of the disk become less defined, suggesting a gradual decrease in stellar density with increasing radial distance from the center. The galaxy does not display any obvious signs of recent major merger events. Overall, the object presents a relatively symmetrical morphology, consistent with a disk galaxy viewed at a high inclination angle.
