The galaxy exhibits a generally smooth morphology. It appears elliptical in shape, with a high degree of central concentration. The color gradient transitions from a yellowish-white core to a slightly redder outer halo. There is no readily apparent spiral arm structure or significant dust lane obscuration. Subtle asymmetries or minor disturbances may exist in the outer regions, though they are not sharply defined. Any tidal features or signs of a major ongoing merger are not obvious within the observational constraints. The light profile suggests that the object is relatively evolved.
