The galaxy presents as a flattened, disk-shaped structure. Its primary orientation is edge-on, revealing a prominent central bulge that appears relatively smooth and rounded. The dust lane, characteristic of many spiral or disk galaxies, is not distinctly visible. The overall color of the galactic disk is a yellow-white hue, possibly indicating an older stellar population. There are some indications of disturbances or minor asymmetries within the galactic structure. No clear signs of a major ongoing merger are observed.
