The galaxy in the image presents a relatively smooth and concentrated morphology. It appears elliptical in shape, with a moderate degree of roundness, showing a transition between a perfectly circular and a more elongated form. There are no prominent features such as spiral arms or a distinct disk structure visible. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions of the galaxy. The galaxy exhibits a reddish-yellow hue, suggesting an older stellar population with a lower rate of ongoing star formation. There is no immediately obvious sign of a major ongoing merger, though minor disturbances cannot be ruled out.
