The galaxy presents as a flattened, disk-shaped structure, oriented nearly edge-on with a slight tilt. A prominent central bulge dominates the galaxy's core, exhibiting a smooth and concentrated luminosity profile. The bulge appears almost boxy, with rounded edges rather than sharp definition. Moving outward from the core, the disk appears elongated, extending significantly on either side of the bulge. This disk shows subtle variations in surface brightness along its length. The integrated light from the galaxy appears relatively redder within the central bulge, transitioning to a bluer hue in the outer disk. The overall morphology does not exhibit any signs of significant tidal disturbances or ongoing mergers. 
