The galaxy presents as a somewhat elliptical, face-on system. The central region exhibits a high surface brightness, appearing nearly stellar in its condensation. Moving outward, the luminosity decreases smoothly and gradually, suggesting a lack of prominent spiral arms or distinct features. There is a faint bluish tinge, especially in the outer regions, indicating the presence of a younger stellar population, or ongoing star formation. The galaxy does not appear significantly disturbed, although some minor asymmetries may be present. No obvious signs of a major merger event are visible. The overall appearance suggests a morphology somewhere between a lenticular galaxy and a spiral galaxy with poorly defined arms. 
