The galaxy presents a morphology consistent with an ongoing or recent merger event. The object exhibits an irregular shape, deviating significantly from a pure elliptical or spiral form.  There is a dominant central component with several apparent bright knots or clumps suggesting multiple centers of luminosity, which likely correspond to the nuclei of the merging galaxies and/or regions of intense star formation triggered by the interaction.

The color gradient indicates a likely evolved stellar population in the central body, with a trend towards bluer colors in the outer components. This color variation suggests a differential age and composition in the different interacting components, with the tidal features likely exhibiting younger stellar populations due to starbursts or infalling material. The relative smoothness of the overall light distribution is disrupted by the noted clumps, but without a clear disk-like structure being apparent. These features support a scenario of galaxy interaction where distinct galaxies are in the process of coalescing and distorting each other gravitationally.
