The galaxy presents a generally elliptical morphology with a smooth, centralized light distribution. A dominant, bright, yellowish core is observed, which decreases gradually in intensity toward the periphery. The extended halo appears relatively smooth, lacking prominent spiral arm structures or significant dust lane features. The overall color profile suggests a population of older stars. No evidence of recent major merger events is apparent, though subtle asymmetries may indicate minor gravitational interactions or disturbances. The galaxy exhibits a moderate size.