The galaxy presents an elliptical morphology with a moderate degree of central concentration. It shows evidence of interaction or a merging event, as indicated by an irregular shape and potential tidal features. The primary body of the galaxy exhibits a smooth light distribution, but there's a distinct secondary luminous component that seems separate from the main body. The galaxy demonstrates a complex color gradient. The central region exhibits a yellow hue, transitioning to a bluer color on one side and a redder tint on the other, possibly indicating variations in stellar populations or dust distribution. There appears to be a disturbed morphology, suggesting a dynamic event, possibly a recent interaction or merger.
