This galaxy presents as an elliptical morphology, displaying a smooth, rounded shape. The light distribution suggests a high degree of radial symmetry. It appears largely featureless, lacking prominent spiral arms or significant dust lanes. The galaxy's core exhibits a high concentration of light, gradually decreasing in intensity towards the outer regions. The observed color suggests a population dominated by older stars, potentially with a lower rate of current star formation. There are no signs of major mergers or tidal disturbances. The galaxy presents a uniform, symmetrical structure.
