The galaxy presents as a relatively smooth, elliptical object, with a high degree of central concentration. Its overall color is a warm yellow, indicative of an older stellar population. The galaxy exhibits a high degree of sphericity, displaying minimal disk-like features. There is no prominent spiral arm structure or dust lane obscuration discernible. The morphology suggests a lack of recent major merger events, appearing relatively undisturbed. There is a subtle color gradient, with the core appearing more yellow and the outer regions showing a slight bluish tint. This subtle color variation could imply a small degree of ongoing or recent star formation activity in the outer regions, though the dominant stellar population appears old. The overall structure implies the galaxy is fairly massive.