The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The color profile suggests a population dominated by older stars, indicated by the redder hues, particularly towards the core. There is a slight color gradient with bluer tones visible in the outer regions, implying the presence of a younger stellar population in these areas, or perhaps residual star formation. The galaxy exhibits a near-perfect elliptical shape, lacking any obvious signs of tidal disturbances, strong spiral arm structures, or recent merger activity. The overall appearance indicates a relatively undisturbed, evolved system.
