The galaxy presents a morphology suggesting an ongoing or recent interaction or merger event. Two distinct luminous cores are visible, indicating the presence of at least two separate galactic nuclei within a single, larger structure. The light distribution is complex and somewhat disturbed, with a notable departure from a smooth, elliptical profile. The overall color of the galaxy is yellowish-white, suggestive of a stellar population that is dominated by older stars, although the presence of some bluer hues in certain regions cannot be ruled out without higher resolution imaging. There are some faint signs of tidal tails or bridges, structures that could be formed by gravitational interactions between galaxies. This galaxy is quite massive, and undergoing moderate star formation.
