The galaxy presents as a largely homogenous, smooth structure. It exhibits a concentrated, centrally bright morphology with a radial decrease in luminosity. The isophotes are generally circular, indicating an elliptical shape with minimal deviation from perfect symmetry. Faint extensions hint at a possible disk or tidal features, although these are not sharply defined. The color is consistent with an older stellar population, showing a redder hue than typically observed in galaxies with active star formation. No distinct spiral arm structure or dust lanes are discernible. The overall appearance is consistent with that of a massive, early-type galaxy at intermediate redshift.
