The galaxy presents an elliptical morphology, appearing mostly smooth in structure with a concentration of luminosity towards the center. It exhibits a generally rounded form, though not perfectly circular. The galaxy shows a warm color profile, indicating a relatively older stellar population and possibly lower current star formation activity. There is a potential interaction or a merger event visible with an object above the galaxy. There is a slight disturbance in the main body. The diameter of the galaxy is a few kiloparsecs. The galaxy's color index suggests it is likely a high-mass system.
