The galaxy presents as a somewhat smooth, elongated structure. It appears to be an elliptical galaxy or potentially a spiral galaxy viewed edge-on. The central bulge exhibits a yellowish-orange hue, which could indicate an older stellar population. The outer regions show a faint bluish tint suggestive of younger stars or ongoing star formation. There is no significant sign of any tidal disturbances or merger activity. The overall morphology seems relatively undisturbed, indicating a dynamically settled system.
