The galaxy presents as an elliptical, relatively smooth object. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the galactic center. The light intensity gradually decreases outwards from the center, showing a diffuse halo surrounding the central region. There's a subtle color gradient visible. The central regions appear bluer than the outer edges, hinting at the presence of younger, hotter stars. No spiral arm structures or distinct dust lanes are readily discernible. Overall, the morphology indicates an evolved system with a substantial spheroidal component and potentially ongoing star formation. There are slight asymmetries indicating a possible minor disturbance event.
