The galaxy presents as an interacting system, displaying clear morphological disturbance. The primary galaxy appears to be an edge-on disk galaxy, characterized by a distinct dust lane traversing its major axis. The bulge appears fairly homogeneous. A second object is near the disk. It presents a more amorphous structure, exhibiting evidence of tidal interactions and potentially ongoing or recent merger activity. There are no strong indications of spiral arm structure in the primary galaxy. The overall color suggests ongoing star formation.
