The galaxy presents as a system undergoing a significant interaction, likely a merger. Two primary luminous components are visible, suggestive of the remnant cores of the merging galaxies. These appear roughly elliptical and are of similar size and luminosity. There is a diffuse, faint envelope of material surrounding the two primary cores, likely composed of stars and gas stripped during the interaction. This envelope appears somewhat irregular, indicating ongoing gravitational disturbances. The galaxy's overall color is relatively uniform, suggesting an older stellar population dominates. The lack of distinct blue regions or knots indicates a low current star formation rate within the system. The overall morphology hints at a late-stage merger, where the distinct structures of the progenitor galaxies are beginning to coalesce.
