The galaxy appears to be a relatively luminous and massive system, exhibiting an elliptical or lenticular morphology. The light profile suggests a smooth, centrally concentrated structure with a high degree of radial symmetry. The isophotes appear generally round, with only slight deviations from perfect circularity. A color gradient is present, with the central regions exhibiting a yellower hue and outer regions displaying a blue tinge. This color difference potentially signifies variations in stellar population age and composition, wherein the inner regions contain older stellar populations and the outer regions contain some younger ones. There appears to be a region of possible minor disturbance or tidal feature located adjacent to it, suggesting past or ongoing interactions with another galaxy. The overall impression is one of an evolved system, residing at moderate redshift.
