The galaxy presents a somewhat disturbed morphology, potentially indicating an ongoing or recent merger event. The primary structure appears largely spheroidal and quite smooth, suggesting an elliptical galaxy. However, the overall shape is not perfectly uniform, displaying some irregularities in the outer regions. There are hints of tidal features and potential secondary galactic components involved in the interaction. The central region exhibits a higher concentration of light, indicative of a dense stellar population, perhaps surrounding a supermassive black hole. The light profile is dominated by redder wavelengths, suggesting an older stellar population and low star formation. There is a component on the lower edge with bluer wavelengths, this could be a region of star formation, a separate galaxy, or a feature in the foreground. 
