The galaxy presents as an elliptical morphology, appearing largely smooth in texture and elliptical in shape. The light profile suggests a high degree of central concentration, fading smoothly towards the edges. The core exhibits a yellowish-orange hue, potentially indicative of an older stellar population. Little to no evidence of spiral arms or active star formation regions are apparent within the observable area. The overall appearance indicates a system nearing the red sequence, potentially with a substantial stellar mass. Faint extensions and small disturbances cannot be ruled out. The galaxy appears relatively isolated.
