The galaxy appears to be in the process of merging, exhibiting a clear dual-core structure. One core displays a bluish hue, indicative of a younger stellar population and potential ongoing star formation. The second core presents a yellower color, suggestive of an older stellar population. The overall morphology is significantly disturbed, lacking any defined spiral arms or elliptical shape. Tidal features, such as faint extensions or distortions, are potentially present suggesting gravitational interaction. The galaxy shows signs of substantial mass, inferred from its overall luminosity and structural complexity. The blue core may indicate a region of enhanced star formation activity. Overall, the system presents a complex interplay of stellar populations and ongoing dynamical processes associated with a galaxy merger.
