The galaxy presents as a dual-component system. The southern component appears to be a spheroidal galaxy, exhibiting a smooth, concentrated light distribution, possibly indicative of an elliptical galaxy. Its color is predominantly white, suggesting an older stellar population with lower levels of on-going star formation. The northern component is more diffuse and bluish in color, indicating the presence of younger stars and active star-forming regions. The two components appear to be interacting, potentially a merger in progress or a close tidal interaction. The overall shape deviates from a simple elliptical or spiral morphology, suggesting a dynamically disturbed system. There is also the suggestion of a tidal bridge of material connecting the two galaxies.
