The galaxy presents a flattened, disk-like morphology, viewed nearly edge-on. The central bulge appears prominent and exhibits a smooth, concentrated light distribution, suggesting an older stellar population. Proceeding outward from the bulge, a distinct dust lane is visible, bisecting the galaxy. This obscuration suggests a significant presence of interstellar dust and gas within the galactic disk.

The visible disk itself appears relatively smooth, with some subtle indications of spiral structure or irregularities. The color gradients suggest varying stellar populations across the galaxy, bluer regions indicating more active star formation. No bright knots or HII regions are clearly discernible, implying a relatively quiescent star formation rate. The galaxy's overall structure suggests a possible ongoing interaction or minor disturbance.
