The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The overall shape appears largely rounded, exhibiting minimal deviation from circular symmetry. There is no immediately apparent evidence of significant tidal features, major disturbances, or ongoing merger activity. The light profile suggests a more evolved system, with a relatively low rate of star formation. The colors are dominated by redder wavelengths, implying an older stellar population. Fainter blue light can be observed with larger radii. The data are consistent with the classification of a massive elliptical galaxy at moderate redshift.
