The galaxy presents as a somewhat smooth, centrally concentrated object with a generally elliptical morphology. A subtle color gradient is visible, trending from a more yellowish-white core to a slightly bluer halo. The central region appears quite bright. While the galaxy lacks distinct spiral arm structures, a mild disturbance or asymmetry cannot be ruled out, but overall the object appears relatively undisturbed, perhaps an early type. Star formation may be present, but subdued. The isophotes gradually fade toward the galaxy's outer regions, suggesting a decreasing stellar density. No obvious signs of a major merger are apparent, as its light appears quite well-mixed and settled.
