The galaxy presents a primarily smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing yellowish-white, indicative of an older stellar population. A surrounding halo or disk is discernible, showing a slight flattening and a bluer hue, potentially suggesting a more recent burst of star formation in the outer regions. There's a subtle indication of minor disturbance or interaction in the galaxy's structure, though no major tidal features or merger remnants are immediately obvious. The overall roundness suggests that it is viewed close to face-on.
