The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, appearing yellowish-white, potentially indicative of a significant population of older stars. Moving outwards from the center, the galaxy's light becomes more diffuse, fading into the background sky. The color shifts slightly towards a redder hue, suggesting a possible gradient in stellar populations or dust content. There's no immediately discernible spiral arm structure or prominent dust lanes. There's a subtle elongation in the galaxy's overall shape. The overall structure appears relatively undisturbed, with no obvious signs of a major ongoing merger event, although a slight asymmetry hints at the possibility of a past interaction.
