The galaxy presents as a relatively smooth object with a concentrated central bulge. Its overall shape appears largely spheroidal, showing a high degree of circularity. There's a subtle color gradient, transitioning from a slightly bluer hue in the central regions, potentially indicating younger stellar populations or ongoing star formation, to a somewhat redder periphery. No prominent spiral arms or distinct disk-like features are readily discernible. The galaxy seems to be relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers, though subtle asymmetries might suggest minor gravitational interactions in its past. Overall, this object visually presents characteristics consistent with an elliptical galaxy at a significant cosmological distance.
