The galaxy presents as an elongated structure, viewed nearly edge-on. A central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. The surrounding disk shows a bluer color, particularly at its extremities, which could indicate more recent star formation. Dark dust lanes may obscure parts of the disk. There are no obvious signs of major tidal disturbances or ongoing mergers, although minor asymmetries cannot be ruled out. The overall shape suggests it is likely a spiral galaxy, possibly of type Sb or Sc, seen at a high inclination.
