The galaxy presents a largely smooth, elliptical morphology. The light profile suggests a concentration of older stellar populations toward the central region, as indicated by the yellowish hue. There is very little evidence of spiral arm structure or dust lanes. The galaxy appears relatively undisturbed with no obvious signs of ongoing major mergers or tidal interactions. Its shape is nearly circular, showing a slight deviation from perfect roundness. The overall form points to an early-type galaxy, likely a lenticular or elliptical galaxy at a moderate redshift.
