The galaxy presents as a single, somewhat diffuse, yellowish-orange object. It exhibits a morphology consistent with a smooth, elliptical galaxy. The shape is largely circular, showing no prominent spiral arm structures or distinct disk features. There appears to be an active or recent merger event underway. The presence of two distinct, though slightly overlapping, bright central regions or nuclei suggest this merger. There is evidence of some tidal distortion in the form of faint extended light surrounding the central body. These features suggest a significant gravitational interaction between the merging components. Overall the galaxy appears to be a relatively massive system with a low star formation rate.
