The galaxy presents an edge-on disk morphology. A prominent bulge, concentrated towards the center, is visible. The bulge appears relatively smooth. Dust obscuration is apparent along the galactic plane, manifesting as a dark lane that bisects the galaxy. The disk component appears thin and elongated. There is a noticeable color gradient, with the bulge exhibiting a yellower, possibly older stellar population compared to the disk. The disk shows hints of fainter, bluer regions, potentially indicative of ongoing star formation.
