The galaxy presents as a merging system of intermediate redshift. The morphology suggests a relatively smooth, elliptical or lenticular galaxy interacting with a smaller, possibly disk-like galaxy. One component exhibits a dominant reddish hue, indicating an older stellar population with reduced recent star formation, while the other component displays a greenish tint which indicates higher levels of star formation. There appears to be some tidal distortion indicative of gravitational interaction. The system's intermediate roundness suggests a transition between a spherical and elongated shape, possibly influenced by the ongoing merger. The light distribution indicates the presence of an extensive halo. Overall, this galaxy is an interacting system undergoing changes in morphology and stellar populations as a result of the merging process.
