The galaxy exhibits a complex morphology, appearing to be in the process of a significant interaction or merger. Two distinct, bright nuclei are visible, separated by a short distance. These nuclei exhibit a yellowish-orange hue, potentially indicating an older stellar population and/or significant dust obscuration.

Extending from one of the nuclei is a plume or tidal tail of bluish light, suggesting the presence of younger, hotter stars, possibly formed during the interaction. This tail extends away from the main body of the galaxy. The overall shape is irregular and disturbed, indicative of gravitational forces disrupting its original structure.
