The galaxy presents as an edge-on spiral or lenticular type, exhibiting a well-defined and elongated disk. The central bulge appears to be relatively small and not particularly prominent, showing a slight, if any, boxy morphology. There is a hint of possible dust lane obscuration along the central plane of the disk, giving the galaxy a slightly non-uniform appearance. The galaxy shows no obvious signs of recent major merger activity or significant tidal disturbances, although minor asymmetries or disturbances cannot be ruled out. The overall color of the galaxy appears relatively uniform across the disk and is not particularly blue, suggesting ongoing but likely not particularly intense star formation.
