The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. It exhibits a centrally concentrated light profile, suggesting a dense stellar population in its core. The isophotes are generally elliptical, with the galaxy appearing moderately elongated. There's a subtle color gradient, with the central region displaying a yellowish hue, possibly indicative of an older stellar population and a relative absence of ongoing star formation. The outer regions appear slightly bluer, which could be due to a small amount of younger stars. There is no apparent active galactic nucleus based on the smoothness and lack of bright, point-source emission at the center. The galaxy shows no signs of major disturbances or tidal features to suggest recent or ongoing merger activity, though a subtle asymmetry could indicate minor interaction in the past. Overall, the galaxy seems to be relatively evolved and quiescent.
