This galaxy presents a somewhat elongated, elliptical morphology. The central region exhibits a bright, concentrated yellowish-orange hue, suggestive of an older stellar population. The outer regions display a bluer, more diffuse color. The smooth appearance implies minimal dust lanes or prominent spiral arm structures are visible in this image, which would mean that there is not much current star formation, though there is some. There is no evidence of a major merger or strong tidal disturbance. It appears to be a relatively undisturbed system, possibly undergoing gradual evolution.
