The galaxy presents as a smooth, elongated elliptical. It exhibits a relatively high degree of central concentration, with the light intensity peaking noticeably towards the nucleus. The outer regions of the galaxy gradually fade into the background sky, lacking any sharp or distinct edges. There appears to be very little to no evidence of spiral arm structure. The galaxy displays a subtle color gradient, with the core appearing slightly bluer than the outer regions, suggesting the presence of a population of younger stars towards the center, although older stars seem to dominate. Overall, it presents as a relatively undisturbed system with minimal signs of recent major mergers or interactions.
