The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, featureless appearance with a highly concentrated central bulge that fades gradually towards its outer edges. The color profile suggests a predominantly older stellar population, indicated by the yellow-red hue, with likely minimal ongoing star formation. There is no discernible spiral arm structure or dust lane obscuration visible. The galaxy appears largely undisturbed, showing no strong signs of interaction or tidal features, suggesting it is an isolated system or has undergone significant relaxation since any potential merger event. The overall morphology points towards a mature galaxy, potentially a lenticular or elliptical type, situated at an intermediate redshift.
