The galaxy presents a largely smooth and rounded morphology. A central bulge, approximately 5 kiloparsecs in radius, exhibits a concentrated luminosity gradient, appearing yellowish-white. There is little evidence of spiral arm structure or significant dust lanes. The galaxy lacks obvious signs of major mergers or tidal disturbances. The overall light profile suggests an elliptical or lenticular type galaxy. Marginal color gradients imply potential variations in stellar populations, but this may also be due to redshift. The absence of blue light implies that the object is most likely quiescent.
