The galaxy presents as a merging system, with two distinct components apparent. The overall morphology is somewhat elongated, deviating from a purely elliptical shape. One component appears more diffuse and slightly more circular, with a smooth light distribution. The second component is more compact and appears brighter, possibly indicating a higher concentration of stars or active galactic nuclei. There may be a faint tidal tail or bridge connecting the two components, suggesting ongoing gravitational interaction. The system is generally yellow, but shows slightly differing color gradients throughout. The overall structure exhibits moderate signs of disturbance, which points to a galaxy that is undergoing tidal disruption due to the ongoing merger.
