The galaxy presents as a system undergoing significant interaction or possible merger, displaying a disturbed morphology. There is a dominant central concentration of light, likely representing the core of one of the progenitor galaxies. A second, smaller concentration of light appears nearby, possibly a smaller galaxy being accreted or a tidal feature resulting from the interaction. The overall color is relatively uniform and leans towards the redder end of the spectrum, suggesting a population of older stars. There is minimal evidence of ongoing, widespread star formation. The galaxy lacks a well-defined spiral structure, indicating that the interaction has disrupted any pre-existing disk morphology. The galaxy appears moderately luminous and relatively massive, based on its apparent size and brightness at its redshift.
