The galaxy presents as a system undergoing a possible merger or significant interaction. It appears to be composed of two distinct, yet closely associated, luminous components. The overall color profile suggests an older stellar population, predominantly yellow-red in hue. One component is brighter and more diffuse, appearing relatively smooth in texture. The other component is slightly smaller, less luminous and slightly more compact. There may be some tidal distortions or faint extensions visible, hinting at gravitational interaction between the two components. Overall, the structure suggests a complex, dynamic system, possibly in the late stages of a merger event with a substantial stellar mass. Star formation appears to be low.