The galaxy presents as a relatively smooth object, though not perfectly spherical, appearing more elliptical in shape. There is a slight elongation, giving it a somewhat cigar-like appearance. Its color suggests an older stellar population. The concentration of light is greatest toward the galaxy's center, gradually decreasing outwards. There are no strong indications of spiral arm structure or distinct features. Minimal signs of any major merger events or significant tidal disturbances are visible, though some minor disturbances cannot be ruled out.
