The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, relatively featureless appearance with a high degree of central concentration. The light profile appears to gradually decrease in intensity from the core outwards. Based on the red, green, and z-band magnitudes, there is a dominance of light in the redder wavelengths, suggesting an older stellar population. There is minimal evidence of spiral arms, disk-like structures, or recent major mergers. The galaxy appears largely undisturbed with a highly symmetrical, round shape. The color distribution is relatively uniform, with a smooth transition between the core and the outer regions. Star formation is likely suppressed. Based on the absolute magnitude values, it is a moderately luminous galaxy at its redshift.
