The galaxy appears to be a complex system, likely undergoing a merging event. There are at least two distinct luminous regions visible, suggesting the presence of multiple galactic nuclei or highly concentrated star clusters. The overall morphology is irregular and somewhat disturbed, with a diffuse, less structured halo surrounding the more compact cores. The color gradient within the galaxy indicates a possible mix of stellar populations; the central regions display a yellowish hue, suggesting older, redder stars, while the outer regions may contain a bluer population indicative of recent star formation. The system does not show strong evidence of a well-defined spiral or elliptical structure, leaning towards an irregular or peculiar classification, possibly influenced by the ongoing interaction. There might be tidal features present in the image. The relative brightness of different components suggests varying densities and stellar populations within the system.
