The galaxy appears to be undergoing a significant interaction or merger. The morphology is highly disturbed, with an irregular shape and no clear spiral arm structure. There appears to be a bright central core with an asymmetric distribution of light. Extended diffuse emission is visible around the main body of the galaxy. There is likely ongoing or recently ceased star formation, indicated by the yellow-orange hue. The features suggest a relatively high rate of star formation. It is possible this is two galaxies colliding, or a single galaxy being disrupted by an interaction with a smaller companion. There is a possible tidal tail or bridge of material extending from the main body.
