The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated distribution of light. The core region exhibits a bright, yellowish hue, suggesting an older stellar population with less ongoing star formation. The outer regions fade in intensity, displaying a gradual decrease in luminosity and a transition towards redder colors. There is very little evidence of spiral arm structure or dust lanes. The overall morphology is largely undisturbed, indicating a lack of recent major merger events. The galaxy is relatively round in appearance. Although it has a high mass, its star formation is extremely low.
