The galaxy appears to be an edge-on spiral galaxy with a prominent bulge. The dust lane is relatively narrow, sharply defined and bisects the galaxy's disk. The disk itself shows a slight warping, with a brighter region on one side compared to the other. There is a smooth appearance to the galaxy, though the dust lane reveals some substructure. The overall color profile suggests an older stellar population, with a moderate concentration of light toward the center and a gradual decline in luminosity moving outwards. No signs of recent major mergers are visible.
