The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of central concentration. The color profile suggests a population of older stars, evident by the yellowish hue of the galaxy's core. There is little indication of active star formation. The galaxy exhibits a well-defined, rounded structure with no major disturbances in its overall shape. The gradual decrease in surface brightness from the core outwards indicates a lack of prominent spiral arms or a distinct disk component.
