This galaxy appears to be undergoing a significant merger event. The morphology suggests a relatively smooth overall structure, but with clear signs of interaction. Two distinct, bright nuclei are visible, indicating the presence of two previously separate galactic cores. The redder hues of the two nuclei, and surrounding tidal features, are indicative of an older stellar population and a dust component. The system does not exhibit a well-defined disk structure. There is evidence of minor disturbances in the surrounding stellar distribution, but the object is also significantly distorted, with a significant amount of mass undergoing a merger. A faint bridge of light is seen in the area between the two main centers of brightness, likely representing stars and gas being stripped during the interaction.
