The galaxy appears to be undergoing a significant interaction or merger. There are two distinct, bright nuclei visible, suggesting two galaxies in close proximity. The larger of the two has a more diffuse, somewhat amorphous shape, while the smaller is more compact and well-defined. There is evidence of tidal features or a bridge of material connecting the two, implying gravitational disturbance. The color profile indicates a mix of stellar populations, with older, redder stars contributing to the overall luminosity, and regions that have bluer hues that could indicate ongoing or recent star formation. The overall morphology suggests a dynamic system far from equilibrium.
