The observed galaxy presents as a smooth, elliptical-like structure. It exhibits a concentrated central bulge with a distinct color gradient, appearing more yellow toward the core, indicative of an older stellar population and reduced star formation. The galaxy appears elongated, with an approximate axis ratio suggesting a non-spherical morphology. There is no visually apparent spiral arm structure or dust lane obscuration. The overall appearance suggests a relatively evolved system, potentially classified as an elliptical or lenticular galaxy at a considerable distance. There is no visible evidence of any major ongoing merger activity, however minor disturbances cannot be ruled out.
