The galaxy appears to be undergoing a merger or significant interaction. Two distinct, bright nuclei are visible, suggesting two galaxies in the process of combining. These galactic centers exhibit a yellowish hue, possibly indicating an older stellar population or dust obscuration. There is some extended, diffuse emission surrounding the two central components, though no clear spiral arms or a well-defined disk structure are apparent. There seems to be some disturbance to the overall structure of the galaxy.
