The galaxy presents as a centrally concentrated system with a generally smooth, elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Progressing outward, the galactic halo diffuses into a fainter, bluer-tinged periphery. The smooth texture of the galaxy's light distribution, combined with the lack of obvious spiral arm structures or dust lanes, implies that this is likely a relatively evolved system. There are slight indications of minor disturbances or tidal features in the outer halo, but it mostly has a undisturbed appearance. Overall, it presents as a relatively undisturbed, elliptical galaxy with minimal ongoing star formation.
