The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, emitting primarily in yellow wavelengths. A gradual decrease in luminosity extends outwards from the core, with the outer regions appearing more diffuse. There is a subtle transition from a brighter yellowish core to a slightly redder, fainter outer halo. No distinct spiral arms or obvious dust lanes are visible. There is no evidence of any major ongoing merger activity or significant tidal disturbances, though subtle irregularities in the outer halo cannot be ruled out completely without higher resolution data. The overall morphology is indicative of an evolved system, possibly with a suppressed star formation rate. The round shape shows it is most likely an elliptical galaxy type.
