The galaxy presents as a largely smooth, elliptical-like structure, with a concentrated central bulge. It exhibits a yellowish-golden hue, suggestive of an older stellar population. There's a subtle elongation, indicating a shape that deviates slightly from being perfectly circular, tending toward a more oblate spheroid. No prominent spiral arms or significant dust lanes are discernible within the observable features. There are no signs of any major merger events, but there is a subtle disturbance in shape. The light profile appears smooth and diffused, fading gradually toward the outer edges. Based on the red color, the galaxy is likely a large, mature system.
