The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated central bulge that gradually diffuses outwards. The light distribution suggests a relatively high Sersic index. The color gradient transitions smoothly from a yellowish-white core to a slightly redder halo, which indicates an aging stellar population within the galactic structure. The overall appearance is consistent with a well-formed galaxy without substantial tidal disturbances or asymmetries, pointing to a lack of recent major merger events. The aspect ratio of the galaxy suggests it's not perfectly spherical, but rather slightly elongated along one axis.
