The galaxy presents as an elliptical or lenticular galaxy type, exhibiting a predominantly smooth morphology. A very faint extended structure could potentially be a disk, but is unlikely. Its color gradient indicates a higher concentration of older stellar populations toward the core, consistent with diminished recent star formation. The galaxy appears isolated with no signs of major mergers or tidal disturbances, suggesting a relatively undisturbed evolutionary history. Overall, this galaxy seems to be a large, relatively quiescent system.
