The galaxy presents as a pair of closely interacting, or possibly merging, elliptical galaxies. Each component exhibits a bright, centrally concentrated core. The light distribution in each galaxy appears smooth and relatively featureless, suggesting an older stellar population and a lack of significant ongoing star formation. Faint tidal features or diffuse stellar halos are tentatively observed around the primary bodies, which may indicate gravitational disturbances resulting from their interaction. A slight color gradient is visible, with the core of each galaxy appearing slightly redder and the outer regions exhibiting a bluer hue. The overall morphology hints at a system undergoing a process of hierarchical assembly, where smaller galaxies are merging to form a larger structure.
