The galaxy appears as a centrally concentrated, smooth object with a generally elliptical morphology. The light profile suggests a relatively featureless structure, dominated by an older stellar population. There may be a subtle disk component, but it is not prominent. The galaxy presents a central bulge and a faint surrounding halo, with a slight elongation along one axis, moving it away from perfectly circular. Color gradients within the galaxy appear subtle; the central region might exhibit slightly bluer hues, potentially indicating a small amount of ongoing, recent, or residual star formation activity, while the outer regions are redder, likely populated with older stars. There does not appear to be any signs of active galactic nuclei activity or significant dust lanes. The overall undisturbed morphology suggests a quiescent system without recent major merger events. The low star formation rate agrees with the older stellar population.
