The galaxy presents as an elliptical morphology, possibly with a central bulge. The color gradient suggests older stellar populations concentrated within the core, with a yellow-white hue emanating from the galaxy's center. There is asymmetry within its disk, suggesting an ongoing interaction or disturbance. Two regions of distorted stars are clearly visible around the galaxy, suggesting a potential merger or tidal interactions. The relatively smooth appearance and concentrated light profile point toward a higher Sersic index. 
