This galaxy exhibits characteristics consistent with a system undergoing a major merger event or displaying significant tidal disturbances. The morphology deviates substantially from a smooth or elliptical profile, revealing an irregular and complex structure. Evidence suggests the presence of at least two distinct nuclei or regions of high stellar density.

The galaxy presents varying colors indicating differences in stellar populations and/or dust content across the system. There are areas of bluish or greenish hues which likely represent regions of ongoing star formation. Additionally, the galaxy exhibits a reddish tint, which may indicate the presence of an older, redder stellar population and/or dust obscuration.

Overall, the system appears to be actively evolving, with probable interactions between multiple components influencing its observed morphology and stellar populations. Further spectroscopic analysis would be needed to confirm these observations.
