The galaxy presents as a fairly symmetrical, centrally concentrated object. Its overall morphology appears elliptical, with a high degree of roundness. The light profile suggests a smooth distribution, lacking any obvious spiral arm structures or prominent dust lanes. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. Progressing outward from the center, the color shifts subtly towards a redder tone. The outer regions display a diffuse, extended halo, fading gradually into the background. There is no evidence of major tidal disturbances or ongoing mergers. Overall, the galaxy appears to be a relatively undisturbed, evolved system, characterized by a dominant, spheroidal component.
