The galaxy presents as a centrally concentrated, luminous object. The morphology appears to be primarily smooth, with a high degree of central light concentration, possibly indicating an elliptical or lenticular galaxy type. There is a hint of disk-like structure, but this is not well defined.

The central region exhibits a yellowish-white hue, suggesting a population of older stars. Progressing outward from the center, a bluish component becomes more prominent, possibly indicative of ongoing or recent star formation in the galaxy's outer regions. The galaxy shows slight signs of disturbance but mostly appears to be relatively isolated.
