The galaxy presents as a relatively smooth, elliptical structure. It exhibits a central bulge that appears bright and concentrated, fading outward into a diffuse halo. The overall color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue, with possibly a slight blue-ish hint towards the outer edges. The galaxy's morphology seems undisturbed, with no obvious signs of recent major mergers or tidal interactions. The shape is predominantly spheroid with some elongation, tending toward a lenticular form. There is a subtle, disk-like structure that can be implied.