The galaxy presents as an interacting system, potentially in the late stages of a merger. It exhibits two primary luminous components. One component is characterized by a relatively smooth, rounded morphology with a concentrated, bright core, suggesting an older stellar population. The second component is more diffuse and elongated, possibly indicating tidal disruption or ongoing star formation activity. The tidal features suggest gravitational interaction between the galaxies. The light in the galaxies appears to be dominated by bluer light. The system appears to be relatively compact, with the two luminous components in close proximity.
