The galaxy presents as an elliptical morphology with a high degree of central concentration. The core is bright and yellow. A fainter disk surrounds the core, with a slight green tinge, indicating the presence of some younger stars or ionized gas within the galaxy. It appears generally smooth with a slight bulge and no significant dust lanes or spiral arm structures are discernible. The galaxy does not appear to be undergoing any major merging activity based on the undisturbed overall shape. It is moderately large with high mass. The star formation rate is low, with some remaining star formation.
