The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It presents an elongated shape, with the light concentrated toward the center. The color gradient transitions from a yellowish central bulge to a redder hue at the outer edges, suggesting an older stellar population concentrated within the bulge. The absence of discernible spiral arms or dust lanes supports its classification as an elliptical. The general smoothness implies that the rate of star formation is subdued.
