The observed galaxy presents as an elliptical morphology, with a smooth, featureless appearance. The central region exhibits a concentration of yellowish light, suggesting an older stellar population. The overall color gradient indicates that bluer, younger stars might be less prevalent and primarily reside closer to the outer edges of the galaxy. The isophotes of the galaxy are somewhat elongated. The galaxy appears undisturbed, showing no significant tidal features or signs of recent mergers. The smoothness of the light distribution is consistent with a well-mixed stellar population.
