The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing as a bright, yellowish-orange core. This core diffuses outward into a less concentrated halo. The halo shows hints of bluer hues, possibly indicative of younger stellar populations or ongoing star formation relative to the core, though this is subtle. There is no clear evidence of spiral arms or a distinct disk structure. Overall, the galaxy appears to be a relatively undisturbed system, showing no obvious signs of recent major merger activity or tidal disruptions. It exhibits a shape ranging from round to slightly elliptical.
