The galaxy presents as a flattened, elliptical shape, appearing elongated along one axis. Its light profile suggests a smooth distribution with a centrally concentrated bulge that fades gradually outward, indicating an absence of strong spiral arm structures or distinct features. The color gradient transitions from a yellowish-white core to a bluer, fainter outer halo. The color profile suggests older stellar populations are centrally concentrated. There may be indications of minor tidal disturbances or interactions, based on faint asymmetries in the halo. These features are not prominent and do not appear to indicate an ongoing major merger. The galaxy shows indications of star formation, with a likely mass of around 10^10 solar masses. The smooth appearance suggests a relatively evolved system. 
