The galaxy appears to be relatively compact, exhibiting a centrally concentrated morphology. It displays a red-shifted spectral appearance. The object is bright and relatively smooth, showing indications of a central bulge component. Indications of disk features are not readily apparent. There also appears to be a nearby merging galaxy. The merger appears to show signs of a significant disturbance, indicated by the lack of a clearly defined galactic shape. The appearance suggests that this system is dynamically active, likely undergoing a merger process.
