The galaxy presents a morphology indicative of an ongoing or recent merger event. Two distinct luminous components are visible, suggesting the presence of two galactic nuclei in close proximity. The larger nucleus exhibits a more diffuse, potentially older stellar population, as evidenced by its yellowish hue. The smaller nucleus appears more compact with a similar color. There is a distorted shape to the overall structure, with tidal features or streams of material faintly visible between the two components. There is a relatively smooth profile suggesting either the merging process is advanced, or that these are elliptical galaxies merging. 
