The galaxy presents as an elongated, disk-like structure, viewed nearly edge-on. A prominent central bulge dominates its morphology. The bulge exhibits a smooth, somewhat rounded appearance and is intensely luminous, radiating a yellowish-white light, suggesting a population of older stars. 

The galactic disk is visible as a faint, flattened structure extending outwards from the bulge. The disk demonstrates a subtle color gradient; reddish tones are observed on one side, possibly indicating regions of dust obscuration or a higher concentration of older stellar populations. The other side of the disk shows hints of greenish light, hinting at the presence of some active star formation.

Overall, the galaxy displays a relatively undisturbed morphology, with no apparent signs of major mergers or significant tidal disruptions.
