The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. The color profile suggests an older stellar population, indicated by the reddish-yellow hue in the central region, becoming slightly bluer towards the outer edges, suggestive of more recent star formation in the periphery. The galaxy appears to be relatively undisturbed, lacking any obvious signs of tidal interactions or ongoing mergers, although a slight asymmetry cannot be ruled out. The isophotes appear mostly regular, with a roundish to slightly elongated shape. There is no prominent disk or spiral structure visible. The overall light distribution indicates a high Sersic index profile, consistent with a spheroid-dominated galaxy.
