The galaxy presents as a flattened, disk-shaped structure, observed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. The disk itself appears relatively smooth and featureless, lacking distinct spiral arm structures. Its color gradients indicate a likely mix of stellar populations, with the outer regions possibly containing younger, bluer stars, though this is difficult to discern definitively. The galaxy's overall morphology points towards it being a spiral galaxy, likely of type Sb or Sc, seen at a high inclination. There is no clear indication of a major ongoing merger event, but the possibility of minor tidal disturbances cannot be completely ruled out. The bulge is generally rounded in shape, not boxy.
