The galaxy presents as an elliptical morphology, appearing elongated with a high degree of axial ratio. It displays a smooth light distribution, exhibiting a gradual change in surface brightness from the center outwards. The core is relatively compact with a golden hue, likely indicating an older stellar population. The outer regions appear fainter with a bluish tint, perhaps from younger stars. No spiral arms or obvious dust lanes are discernible. The galaxy doesn't show any signs of major tidal disturbances or ongoing merger events. The overall structure is suggestive of an evolved system undergoing relatively low levels of star formation.
