The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a smooth, concentrated central region with a slightly elongated morphology. The core displays a yellowish-orange hue, suggestive of an older stellar population. Surrounding this core is a more diffuse halo of bluish light, potentially indicating the presence of some younger, hotter stars, or possibly reflecting dust. There appears to be no discernible spiral arm structure or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of major tidal distortions or ongoing mergers.
