The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The overall color appears somewhat redder compared to other objects in the field of view. There are no clear spiral arm structures or dust lanes visible. The galaxy appears to be isolated with no major signs of ongoing merger activity or significant tidal disturbances. It displays an oblate morphology, being quite round, as opposed to having an elongated shape. The galaxy is characterized by a substantial stellar mass. It exhibits very low levels of ongoing star formation.
