The galaxy appears as a faint, elongated object, suggestive of a disk galaxy viewed at a high inclination. It is relatively small. The light is generally smooth and uniform across the visible structure. The slight color variations suggest subtle differences in stellar populations or dust content within the disk. There is no clear evidence of a central bulge, spiral arms, or any significant ongoing merger activity. Overall, the galaxy presents a generally undisturbed morphology, without obvious signs of recent interactions or starburst activity.
