The galaxy appears to be part of a gravitationally interacting pair. The larger galaxy exhibits a disturbed morphology, with an elongated shape oriented approximately diagonally in the image. The nucleus of this galaxy is bright and concentrated, with the surrounding stellar population appearing yellowish-red. This suggests an older stellar population dominates the galaxy. Faint tidal features are observed, extending away from the galaxy's primary structure, hinting at ongoing or recent interaction with the smaller companion galaxy. The smaller galaxy also possesses a bright, compact nucleus and a similarly reddish color. It is less well defined. A distortion is apparent in this galaxy's shape. The overall color profile of both galaxies suggests a relatively low rate of current star formation.
