The galaxy appears to be in the process of a major merger, displaying significant morphological disturbance. Two distinct galactic nuclei are visible, one with a distinctly bluer color, indicative of younger stellar populations or enhanced star formation, and the other with a redder hue, which could indicate older stars or significant dust extinction. The shape of the overall structure is highly irregular and elongated, deviating significantly from a typical elliptical or spiral morphology. There is some evidence of tidal tails or disrupted material extending from the main body of the galaxy, further supporting the ongoing merger process. The light profile seems relatively smooth, especially considering the disturbed nature of the object, indicating the presence of an older stellar population throughout the system. There is a strong possibility that the galaxy is undergoing a phase of intense star formation activity and may evolve into an elliptical or lenticular galaxy.
