The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse appearance. There is little to no visible substructure such as spiral arms or a prominent bar. The color appears generally uniform across the galaxy, with a slight color gradient towards the center, with the inner region trending towards bluer hues and the outer regions appearing redder. This suggests that the inner region contains slightly younger stellar populations compared to the older, redder stars on the outskirts. The overall roundish morphology indicates a system that is close to being viewed face-on. There is no indication of any major merger events or significant tidal disturbances affecting the overall structure. The absence of a well-defined disk, combined with its smooth appearance, suggest this is likely to be an elliptical galaxy or a lenticular galaxy observed at low resolution.
