The galaxy presents as a merging system. Two distinct luminous cores are visible, each appearing roughly elliptical, suggesting the remnants of two interacting galaxies. The larger core displays a more diffuse, less defined structure, with a smoother overall appearance. In comparison, the smaller core appears more compact and well-defined, but more disturbed. The system exhibits a yellow-red hue, suggestive of an older stellar population and diminished recent star formation. There may be some tidal features or distortions in the system, but the limited resolution makes it difficult to determine their exact nature. The overall morphology suggests an intermediate stage of a galactic merger, where the progenitor galaxies are still distinguishable but significantly influenced by gravitational interaction.