The galaxy presents as a lenticular or possibly an elliptical galaxy with a flattened, disk-like structure. The core region exhibits a significantly higher surface brightness, appearing as a concentrated, yellowish-white bulge. Moving outward from the bulge, the galaxy transitions to a fainter, more diffuse halo or disk. This outer region displays a bluish tint, hinting at the presence of a younger stellar population compared to the core. The galaxy's morphology suggests it is relatively undisturbed, with no apparent signs of major mergers or tidal interactions. The light distribution is smooth and centrally concentrated, consistent with a galaxy that has largely completed its star formation.
