The galaxy presents an overall elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region appears bright and yellowish, suggesting a population of older stars. The outer regions display a gradual decrease in luminosity, with a slightly bluer hue compared to the core. There is a hint of a possible disk structure, but it is not sharply defined. The galaxy does not show any signs of major mergers or tidal disturbances. Overall, the galaxy appears relatively isolated and undisturbed.
