The galaxy presents as a largely smooth, elliptical structure, exhibiting a high degree of radial symmetry. The light profile suggests a centrally concentrated bulge, transitioning smoothly to a more diffuse halo. The color gradient indicates a yellowish-white core, possibly indicative of an older stellar population and/or dust obscuration. Fainter, bluish extensions appear in the galaxy. There are no prominent spiral arm structures or distinct dust lanes visible. The galaxy does not show strong morphological signs of ongoing major merger activity, though there may be some minor disturbances present that could be signs of a recent merger. The overall appearance aligns with that of an early-type galaxy with moderate mass.
