The galaxy exhibits a moderate redshift, suggesting a considerable distance. The morphology appears to be that of a system undergoing a merger. The light profile indicates a generally smooth structure with some distortions. Two main clumps of luminous matter are visible, with a fainter bridge of light connecting them. One of the clumps appears more diffuse than the other. The overall shape is elongated, possibly indicative of tidal interactions. Subtle color variations are present across the galaxy, with bluer regions potentially indicating areas of recent star formation, and redder regions possibly indicative of older stellar populations. Based on the light distribution and structure, the galaxy may be in the later stages of a merger.
