The galaxy presents a generally smooth morphology. The light is concentrated centrally, with a gradual decrease in intensity towards the outer regions, suggesting a higher density of stars and gas in the core. Its elliptical shape deviates slightly from a perfect circle. There are no well-defined spiral arms or a prominent bar structure that can be identified. Faint, diffuse structures or minor disturbances appear within the surrounding halo of the galaxy. The overall color profile indicates a population of older stars, with a bluer hue in the very center which suggests some presence of younger stellar populations or star forming regions. There is no obvious, extremely bright active galactic nucleus, nor are there any distinctive features indicative of a recent major merger event.
