The galaxy presents as a centrally concentrated elliptical or lenticular type. It exhibits a smooth, diffuse morphology with a high degree of radial symmetry. The color gradient indicates a likely dominant population of older stars. There is little to no evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions. Faint color variations may indicate some degree of inhomogeneity in stellar populations, but further spectroscopic analysis would be required to confirm.
