The galaxy presents as a smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile that fades gradually towards the edges. The galaxy's color gradients indicate a population of older stars dominating the central region, displaying a redder hue. The outer regions suggest the presence of a younger stellar population, exhibiting a slightly bluer color, indicating ongoing, albeit minimal, star formation activity. The overall appearance is of a well-formed, isolated system with no visible signs of tidal interactions or major disturbances. The elongation suggests it is not perfectly spherical, but rather more ellipsoidal in shape. There are no prominent dust lanes or spiral arm structures visible.
