The galaxy presents as an edge-on spiral, exhibiting a prominent central bulge with a bright, concentrated luminosity indicative of a high stellar density. The disk component is visible, though highly inclined, and appears significantly flattened, with a length extending approximately twice its width. Faint, diffuse regions of star formation or dust lanes are weakly apparent along the edges of the disk, contributing to a slightly mottled appearance. The overall color profile suggests a population mix of older, redder stars concentrated within the bulge, transitioning to bluer, younger stars within the disk. The galaxy lacks any significant signs of tidal disruption or major ongoing mergers. There is a subtle boxy morphology to the bulge.