The galaxy appears to be a relatively smooth, rounded structure with a concentrated central bulge. There is little evidence of spiral arms or a well-defined disk. The galaxy exhibits a color gradient, transitioning from a bluish-white hue in its core to a reddish-yellow tinge in its outer regions. This suggests a possible difference in stellar populations, with potentially younger, hotter stars concentrated in the center and older, cooler stars dominating the periphery. There is no strong evidence of ongoing major mergers or significant tidal disturbances. The general morphology points towards an elliptical galaxy, possibly in the early stages of its evolution or a lenticular galaxy with a prominent bulge.
