The galaxy presents as a disk galaxy, observed nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk, though viewed at a high inclination, displays a flattened structure. It shows hints of dust lanes or patchy structures within the disk, though the image resolution limits detailed analysis. There appear to be no signs of recent major merger events. The disk's edges fade out gradually, indicating a diffuse distribution of stars and gas.
