The galaxy presents a largely featureless appearance, dominated by a smooth, spheroidal morphology. Its color profile suggests an evolved stellar population, with a central concentration of older, yellowish stars. There is a faint, diffuse halo surrounding the brighter core, indicative of a low-level ongoing star formation or remnants of past star formation events. No prominent spiral arms or dust lanes are discernible. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or mergers affecting its structure. The rounded shape indicates the galaxy is likely an elliptical galaxy with a small disk fraction.