The galaxy presents as a single, centrally concentrated light source. Its morphology appears smooth and relatively featureless, with a roughly elliptical shape that is somewhere in between round and elongated. The galaxy exhibits a color gradient, transitioning from a yellowish core to a bluish outer halo. There is no indication of spiral arms or a defined disk structure. Based on the color and smooth morphology, this could be an elliptical or lenticular galaxy. The relative color differences imply a distribution of stellar populations, with the bluer halo possibly indicative of ongoing or recent star formation relative to the older, redder stellar populations in the core. There are indications that this galaxy may be experiencing a minor merger as there appears to be slight disturbances in shape. 
