The galaxy presents as a largely smooth, elliptical-type structure with a high degree of central concentration. Its overall color appears slightly redder in the observed spectrum. The morphology indicates a system that is well-formed, displaying a near-circular shape. There is no visible evidence of significant tidal disturbances or ongoing mergers, suggesting that it has been relatively isolated or undisturbed for a considerable period. The galaxy appears to have a relatively high mass, and a low star formation rate.
