The galaxy presents as a flattened disk viewed nearly edge-on. A prominent central bulge is observed, appearing smooth and concentrated. There is evidence of a faint, extended halo surrounding the central structure. Dust lanes appear to be present, running along the equatorial plane of the disk, obscuring some of the light from the bulge. The overall color of the galaxy suggests a mix of stellar populations. There is evidence of star formation activity, particularly in the disk, indicated by blue-ish light emission. The galaxy appears relatively undisturbed with no major signs of tidal interactions or mergers. The morphology suggests a spiral galaxy, most likely an Sa or Sb type.
