The galaxy presents as a singular, extended object with a noticeable asymmetry. While a definitive classification is challenging given the image resolution, the galaxy appears to be in a late stage merger with a smaller body. The primary galaxy exhibits a smooth, elliptical morphology, with a bright, concentrated core. A distinct tidal tail or plume feature extends outwards, suggesting gravitational interaction. The color gradient shows a central concentration of yellow and redder hues, potentially indicating an older stellar population. There are hints of ongoing or recent star formation concentrated in one area with bluer hues in the system, although dust obscuration is a possibility that cannot be ruled out. Overall, the galaxy seems to have a significant mass, based on its luminosity.
