The galaxy presents as a moderately bright, elliptical-shaped object with a relatively smooth light distribution. The central region exhibits a more concentrated brightness, suggestive of a bulge. A color gradient is perceptible, transitioning from a yellowish core to slightly bluer outer regions, hinting at potential variations in stellar populations or dust content across the galaxy. There is a lack of clearly defined spiral arms or prominent dust lanes, further supporting its classification as an elliptical galaxy. Its overall morphology suggests a system with a significant fraction of older stellar populations.
