The galaxy presents as a fairly smooth, rounded object. Its core exhibits a bright, concentrated luminosity, indicative of a substantial stellar population. The galaxy's color gradient transitions from a yellowish-white center to a more diffuse, greenish-yellow periphery. There is no clear spiral arm structure or bar feature visible, suggesting it may be an elliptical or lenticular type galaxy. Minor irregularities are present in its outer regions, implying possible past interactions or mergers with smaller galaxies, although the overall morphology appears largely undisturbed. The relatively compact size of the galaxy and its high central brightness point towards a high-mass system with moderate star formation activity. 
