The galaxy appears to be a system undergoing a merger or interaction. The primary component presents a largely spheroidal morphology, exhibiting a smooth, diffuse light distribution. Evidence of tidal features or distortions are present, indicating gravitational interaction. Within the system, there are blue regions showing active star formation. Based on color, the galaxy is a massive system with a stellar mass on the order of 10^10 solar masses. Its star formation rate is relatively low, implying that the active star formation may be subsiding. There is no spiral structure and the red color, therefore, the galaxy appears to be an elliptical galaxy.