The galaxy appears to be a relatively compact, elliptical system. Its core presents a concentrated and luminous region with a yellowish-orange hue, suggesting an older stellar population dominates the central regions. The light fades gradually from the core to the outer regions, which exhibit a fainter, bluish color. The smooth light profile and lack of defined spiral arms or prominent dust lanes imply a morphological type consistent with an elliptical galaxy. There are no obvious signs of major ongoing mergers or strong tidal disturbances, indicating that the galaxy is a relatively undisturbed system. The galaxy shows a slightly elongated shape.
