The galaxy presents a primarily smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. There is a slight elongation observed, with the major axis extending in a northwest-southeast direction. The overall color gradient transitions from the yellowish-white core to a slightly redder halo. Evidence of any significant spiral arm structure or active star formation regions is absent. The galaxy appears relatively undisturbed, with no visible signs of recent mergers or tidal interactions.
