This galaxy appears to be undergoing a merger. Two distinct luminous regions are observed, one more circular and bright, and the other more elongated and less intense in luminosity. The colors of the regions are noticeably different. The brighter region exhibits a pinkish-white hue, suggestive of hotter, younger stellar populations. The more elongated region appears yellowish, potentially indicating older stellar populations or significant dust obscuration. There is some indication of a faint tidal tail extending away from the main bodies of the galaxy, though more data would be needed to confirm this. Overall, the system exhibits morphological disturbances consistent with an ongoing or recent interaction.
