The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge with a gradual decrease in luminosity towards its outer regions. There's a subtle color gradient detectable from the central region to the outer areas, with a yellowish core transitioning to redder hues in the extended halo, indicating older stellar populations at greater radii. The overall symmetrical shape suggests the galaxy is not undergoing major disruptive interactions, although some subtle irregularities could be present. The light distribution suggests a relatively evolved system with low current star formation activity. 
