The galaxy appears to be undergoing a significant interaction or merger. There are at least three distinct luminous regions visible, with a central, brighter component exhibiting a slightly smoother morphology. The other regions are more compact and less defined, possibly representing separate galaxies in the process of merging or tidal features resulting from gravitational interactions. 

The galaxy exhibits a color gradient, with bluer hues concentrated within the central region. This suggests ongoing or recent star formation in the core. Redder colors are observed in the surrounding components, which may indicate older stellar populations. The overall shape is irregular and disturbed, further supporting the evidence of an ongoing merger event. The system is neither perfectly smooth, nor does it appear to be fully disrupted.
