The galaxy presents as a relatively smooth, elliptical structure. The light profile suggests a concentration of stars toward the center, exhibiting a bright, yellowish core. Moving outwards, the light becomes more diffuse with an extension of light reaching about 7 kpc from the center. There is a slight indication of a disk like structure, but the features are not well defined. A possible minor disturbance is detected in the outskirts of the galaxy. The system appears to be a mature galaxy with a significant stellar mass and low star formation.
