The galaxy presents as a somewhat rounded, singular object. Its core exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. The outer regions display a reddish-orange coloration, potentially indicating the presence of dust lanes or regions of older, redder stars. The overall appearance is generally smooth, with little discernible structure or spiral arm features visible. The galaxy does not exhibit signs of a major merger event, though minor disturbances cannot be ruled out.
