This galaxy appears as a luminous, centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish-white hue, suggesting an older stellar population dominating the galactic center. The light gradually diffuses outwards, with the outer regions appearing fainter and slightly redder. No distinct spiral arms or prominent dust lanes are visible. The overall shape is approximately round, with a very subtle elongation that could indicate a slightly ellipsoidal structure. There are no visible signs of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed. The colors indicate a likely evolved stellar population, possibly associated with a lenticular or early-type galaxy.
