The galaxy presents as a relatively compact object. Its overall morphology appears predominantly smooth. A small percentage of the object displays features possibly indicative of a disk, while a high fraction of the object seems smooth. The galaxy exhibits a generally round shape, with only a slight deviation toward an elongated form. There is no strong visual evidence suggesting a major merger is underway, but minor disturbances can be noted in the object's features. The object appears relatively massive, with a moderate star formation rate.
