The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge that is more luminous than the outer regions. The light distribution appears relatively uniform with minimal discernible substructure within the disk or halo. The color profile indicates a yellow-red hue, which suggests a stellar population of older, redder stars and relatively low ongoing star formation. Based on its round shape and low star formation rate, the galaxy is most likely an elliptical galaxy that has undergone significant evolution. There is no sign of any major merging events. 
