The galaxy presents as an elliptical or lenticular type, characterized by a smooth, centrally concentrated light distribution. The galaxy exhibits a subtle color gradient, transitioning from a slightly redder core to a somewhat bluer outer halo.  There is no discernible spiral arm structure or distinct dust lanes apparent in this observation. The galaxy appears relatively undisturbed, without major signs of tidal interactions or recent mergers, although a minor disturbance cannot be ruled out.  The shape is moderately elliptical, departing slightly from a perfectly circular morphology. The galaxy appears to be a large system. The overall visual impression is that of a mature galaxy with an older stellar population, and an attenuated star formation rate.
