This galaxy presents a smooth, elliptical morphology. The light profile suggests a concentrated central bulge that gradually fades into an extended halo. The object appears to be in between round and cigar shaped. There is little to no evidence of spiral arm structure or dust lanes. The galaxy exhibits a yellowish-red hue throughout, indicative of an older stellar population with reduced current star formation. Faint irregular structures or minor disturbances can be observed, suggesting the possibility of a past interaction or merger event.
