The galaxy appears as an elliptical or lenticular structure with a concentrated, bright central bulge. The overall color profile indicates an aging stellar population, with a dominant yellowish hue. The galaxy exhibits a relatively smooth morphology with a high degree of rotational symmetry; however, there are possible minor signs of disturbance, indicated by the very faint asymmetrical extensions around the central region of the galaxy. There may be the presence of an evolved stellar population with suppressed star formation activity.
