This galaxy presents a largely smooth morphology, exhibiting a spheroid-like structure with a high degree of central concentration. The light profile suggests a well-defined core region that gradually fades into the outer regions of the galaxy. The overall color appears to be on the redder side, indicating an older stellar population. There's no obvious presence of strong spiral arms or a prominent disk. There is a subtle color gradient from the inner regions which appear to be a slightly yellow hue, towards the outskirts which exhibit a somewhat bluer tone. The smoothness of the galaxy is consistent with it potentially being an elliptical galaxy or a lenticular galaxy viewed face-on. There is no clear evidence of any major merging events, although subtle disturbances might be present.
