The galaxy exhibits a complex morphology, appearing as a gravitationally interacting system. A larger, primary component displays a relatively smooth, diffuse light profile, suggesting an elliptical or lenticular morphology. This primary component is slightly elongated, but not significantly cigar shaped. A fainter, secondary component is visible in close proximity, potentially a satellite galaxy or tidal dwarf galaxy. There is a strong indication of ongoing or recent merging activity. The overall color is moderately red, implying an older stellar population with ongoing star formation. The system displays moderate disturbance.
