The galaxy presents a complex morphology indicative of an ongoing or recent merger event. It exhibits a disturbed structure, with at least two distinct nuclei or regions of concentrated light, suggesting the interaction of two galaxies. These nuclei appear yellowish in color. 

One nucleus is brighter and slightly more extended than the other. Diffuse tidal features are also visible, extending outwards from the main bodies, possibly indicating tidal tails or disrupted stellar streams resulting from the gravitational interaction. These features are faint and somewhat blue in color.

Overall, the galaxy appears to be luminous, with colors suggesting a stellar population consisting of a mix of old and young stars. The presence of tidal features, combined with the multiple nuclei, strongly indicates that this galaxy is undergoing a significant dynamical interaction.
