The galaxy appears to be an elliptical, exhibiting a smooth, concentrated morphology. It presents a slightly elongated shape, deviating from a perfect circle. There is some evidence of a minor disturbance to its structure, as there is a slight distortion in its overall form. The galaxy has a notable luminosity gradient, appearing brighter towards its core and gradually fading outward. Color analysis indicates a predominantly red hue, suggesting an older stellar population. Based on its observed properties, the galaxy is likely a massive, relatively quiescent system with ongoing but low-level star formation.
