The galaxy presents a largely smooth and rounded morphology, indicative of an elliptical galaxy. It exhibits a concentration of light towards its center, suggesting a prominent galactic nucleus or bulge. There is very little evidence of spiral arm structures or significant dust lanes. The color gradient reveals a central yellowish-white hue, which gradually transitions to bluer tones in the outer regions. This color difference may be due to younger stellar populations existing in the outer regions compared to the center. There is no visual indication of any major ongoing merger events. The overall appearance suggests a relatively evolved galaxy with a dominant smooth component.
