The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the center, the light gradually fades and reddens, indicating potentially cooler stellar populations, dust obscuration, or a change in stellar metallicity within the galaxy. The overall structure appears relatively undisturbed, with no obvious tidal features or major asymmetries that would suggest recent or ongoing merger activity. There is little evidence of spiral arms or distinct disk features. Based on the colour and morphology, it is likely an elliptical galaxy at intermediate redshift.
