The observed galaxy appears as a generally smooth, elliptical-like structure. It exhibits a somewhat round morphology. There is a slight color gradient visible, with the central region appearing more yellow or orange. A fainter secondary object can be seen next to the galaxy that shows hints of redness. Given the overall appearance, the galaxy likely has a high fraction of older stellar populations. The galaxy appears to be relatively undisturbed and not currently undergoing any major merger events.
