The galaxy appears as a slightly elongated, elliptical-like structure. Its core exhibits a concentrated, bright, yellowish-white luminosity, suggesting a population of older stars. Moving outward from the core, the light gradually diffuses, transitioning to a more reddish hue in the outer regions, which could indicate a diminishing population of younger, bluer stars and an increased presence of older, redder stars. The galaxy displays a relatively smooth texture, with no prominent spiral arm structures or significant dust lanes readily apparent in this image. There is a slight hint of asymmetrical morphology, but the bulk of its light is consistent with a reasonably relaxed, relatively undisturbed system. The estimated size of the galaxy would make it smaller than our own Milky Way galaxy. Its color suggests that star formation may be actively occurring, but is minimal and occurring slowly within the system.
