This galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. The overall light distribution appears disturbed, lacking a single, well-defined nucleus. There are multiple apparent luminosity peaks with concentrations of light, suggesting the presence of interacting galactic nuclei or dense star-forming regions. 

The color gradients indicate a mix of stellar populations. The dominant color is reddish-yellow suggesting an older stellar population. Some regions display hints of bluer colors, possibly indicating areas of more recent star formation, perhaps triggered by the interaction. The overall smoothness suggests the late stages of a major merging event.
