The galaxy presents as an elliptical morphology, exhibiting a smooth, spheroidal shape with a bright, concentrated central bulge.  The luminosity gradually decreases from the center outwards, lacking prominent spiral arms or distinct features.  The color profile suggests an older stellar population, with a yellowish-red hue dominant in the core region. There is subtle evidence of bluer regions in the outer halo. The overall appearance indicates a system that is relatively undisturbed with no major ongoing mergers or tidal distortions.  The galaxy appears to be transitioning with signs of some ongoing star formation in its halo.
