The galaxy presents as a merging system, displaying a disturbed morphology with noticeable tidal features. There are multiple nuclei, which suggest that the galaxy is undergoing or has recently undergone a merger event. The main body of the galaxy exhibits a complex structure, lacking a clear spiral arm structure or defined elliptical shape. The color gradient suggests a mix of stellar populations, with the central regions appearing more yellow/red, potentially indicating older stellar populations or dust obscuration. Outward from the center, a bluer component hints at ongoing star formation. The size is moderately large, with significant spatial extent indicative of a developed stellar distribution. The overall luminosity implies a massive system. Evident disturbances in the galaxy’s structure, possibly due to gravitational interactions, appear to be the dominant characteristic of this system.
