The galaxy presents as an edge-on spiral, or possibly lenticular, system. A prominent central bulge dominates the overall structure. This bulge exhibits a yellowish-orange hue, suggesting an older stellar population and diminished star formation within the nuclear region. The disk component is less distinct but appears to be significantly flattened and elongated, supporting the edge-on classification.

The disk shows a fainter, bluer tint compared to the bulge, indicating the presence of younger stars and ongoing, though perhaps moderate, star formation. There is no easily noticeable dust lane bisecting the galaxy. The overall morphology appears relatively undisturbed, showing no strong signs of a recent major merger event. Close inspection hints at some very slight structural asymmetries in the outer disk, but these are subtle and could be due to minor interactions or internal dynamics.
