The observed galaxy exhibits a morphology indicative of a merging system. It appears as a dual-core structure, with two distinct, bright nuclei. The general shape of the galaxy is largely rounded. The presence of the two nuclei suggests a recent or ongoing merger event between two galaxies of comparable size. There is some evidence of possible tidal distortion, although the smoothness of the overall structure may indicate that this is a late-stage merger with the tidal features obscured. Color gradients appear subtle across the body of the galaxy, potentially indicating relatively uniform stellar populations. Further spectroscopic analysis would be needed to fully confirm the nature of the merging components.
