This galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population dominating the central region. The overall morphology appears to be elliptical, with a slight elongation along one axis. The outer regions fade gradually into the background, suggesting a lack of prominent spiral arms or distinct features. There is faint blue tinging on the periphery of the galaxy, which suggests the presence of younger stars on the outskirts. No signs of strong tidal disturbances or merger activity are immediately apparent from visual inspection, but the presence of minor disturbances cannot be ruled out due to the resolution of the image. Overall, the galaxy seems to be a massive elliptical system with an ongoing, low level of star formation.
