The galaxy presents as a relatively smooth, elongated structure, suggesting a possible elliptical morphology or a disk galaxy viewed edge-on. It exhibits a color gradient, appearing slightly bluer toward one end. The galaxy does not show any obvious signs of recent major merger activity or significant tidal disturbances based on its apparent structure. There is a hint of a central concentration, though the resolution is insufficient to determine the presence of a distinct nucleus. Overall, the galaxy seems to be a fairly quiescent system.
