The object presents as a galaxy viewed nearly edge-on. A prominent central bulge appears bright and yellowish-white in color. Dust lanes are subtly visible along the galactic plane, particularly near the bulge, creating some obscuration. The disk component appears relatively thin and extends significantly beyond the central bulge, with a bluish tint, potentially indicating the presence of younger stellar populations and ongoing star formation within the spiral arms, though no distinct spiral arm structure is discernible given the edge-on orientation. The galaxy exhibits a moderate degree of smoothness, but also some subtle features. The overall structure suggests a rotating disk galaxy with a prominent central bulge. There does not appear to be any substantial merging or major disturbance events occurring, with only minor irregularities in the outer regions of the disk.
