The galaxy appears to be undergoing a significant merger event, with the primary component showing a bright, somewhat smooth central region. There seems to be a secondary core or large clump of material slightly offset from the primary center, indicating either a recent capture or a late stage merger.

The galaxy displays an irregular overall shape, lacking clear spiral arms or a well-defined elliptical structure. There is evidence of tidal distortion, potentially in the form of faint extensions or bridges of material, which are more pronounced on one side than the other.

The color profile suggests a generally older stellar population, with a yellow/red hue dominating the core regions, although the color varies across the merging system. Patches of bluer color may be present, potentially indicating regions of more recent star formation triggered by the interaction.
