The galaxy presents as a somewhat elliptical, centrally concentrated object. The core region exhibits a bright, yellowish-orange hue, indicative of an older stellar population. The outer regions display a subtle fading in intensity, transitioning to a more diffuse, slightly redder color, possibly indicating the presence of a moderate amount of dust and/or a population of cooler stars. There is no strong evidence of spiral arm structure or significant morphological disturbances. The overall impression is that of a relatively smooth, early-type galaxy.
