The galaxy appears to be undergoing a significant merger event. Two distinct luminous components are visible, with the primary component appearing somewhat more concentrated and slightly elongated. The secondary component presents a less defined structure. A faint bridge of material seems to connect the two components, suggesting gravitational interaction. Overall, the galaxy exhibits a reddish hue, potentially indicating a population of older stars and/or significant dust obscuration. The system's morphology is highly disturbed, indicative of ongoing tidal forces. There's a hint of irregularity in the outer regions, possibly shredded material being pulled away from one or both of the progenitor galaxies. The core regions appear relatively bright, suggesting ongoing star formation or active galactic nuclei, although this cannot be confirmed solely from this image.
