The galaxy presents as an elliptical morphology, appearing largely smooth and relatively round in shape. The core exhibits a concentrated and bright yellowish-white luminosity, suggesting a substantial population of older stars. The galaxy appears to lack prominent spiral arm structures or significant dust lanes. There are subtle color gradients moving outward from the center; the outer regions appear redder, possibly indicating an aging stellar population compared to the core. Overall, the galaxy shows no obvious signs of major mergers or significant tidal disturbances. The faintness of the outer regions suggest a low star formation rate.
