The galaxy presents as a flattened, disk-like structure, oriented edge-on relative to our line of sight. A prominent central bulge is visible, exhibiting a smooth, concentrated appearance. The bulge displays a yellowish-orange hue, suggestive of an older stellar population with diminished recent star formation.

The disk component appears relatively thin and extends outward from the central bulge. The disk exhibits a bluer tint compared to the bulge. Some patchy regions or subtle undulations are visible within the disk, possibly indicating spiral arm structures viewed edge-on, or areas of ongoing star formation. The overall luminosity profile appears to decrease smoothly from the central bulge outwards along the disk.

The galaxy appears relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers with other large systems. There may be evidence of a minor interaction or slight asymmetry.
