The galaxy presents as a centrally concentrated, smooth elliptical. There is little evidence of spiral arm structure or significant dust lanes. The core exhibits a bright, yellowish-orange hue that diffuses outwards. The outer regions appear fainter, displaying a subtly bluer tinge. The overall morphology suggests a relatively evolved stellar population with a limited rate of ongoing star formation. The lack of significant disturbances indicates that the galaxy is likely not undergoing a major merger event, although a minor interaction cannot be completely ruled out. The object is well-defined and roughly spheroidal in shape, though a slight elongation is detectable.
