The galaxy presents as a fairly smooth, elliptical structure with a high degree of central concentration. Its overall shape is more in-between round and elliptical rather than perfectly circular or elongated. There is little evidence of spiral arms or disk-like features. The galaxy appears to be relatively undisturbed, lacking significant signs of ongoing or recent major merger activity. A very slight asymmetry or minor disturbance might be present in its outer regions, hinting at a possible past interaction or minor merger. The galaxy's color indices indicate it is a red galaxy, implying an older stellar population.
