The galaxy presents as a complex system, likely undergoing a significant interaction or merger. It exhibits a disturbed morphology, deviating from a regular elliptical or spiral structure. Two distinct, bright nuclei are observed, suggesting either a recent merger of two separate galaxies or a galaxy with a highly active galactic nucleus and a prominent star-forming region. A faint tidal tail or bridge of material appears to connect the two nuclei, indicative of gravitational interaction. The overall color of the galaxy appears relatively red, which could indicate an older stellar population with less ongoing star formation. The shape is generally round, but with noticeable disturbances and extensions resulting from the ongoing interaction. There appear to be some minor regions of ongoing star formation present as indicated by the slight blue tint in areas around both nuclei.
