The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be predominantly spheroidal, though it is not perfectly round. It is somewhere in between a round and in-between shape. There are minimal signs of significant disturbance or ongoing major merger activity. Some subtle asymmetry might suggest minor interaction or internal activity, but this needs further investigation. The galaxy exhibits a colour gradient, appearing more blue/green in the central regions, transitioning to redder hues further outwards, indicative of varying stellar populations and potentially ongoing, low-level star formation. The apparent luminosity suggests it is a massive galaxy.
