The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated brightness profile, appearing nearly circular in shape. A faint, diffuse halo surrounds the brighter central region. Color gradients are subtle, but a slight bluish hue is visible in the inner regions, possibly indicating recent or ongoing star formation. There is no evidence of a pronounced disk structure or spiral arms, nor of any major tidal disturbances or ongoing mergers. The galaxy appears relatively undisturbed, with a well-defined and regular structure. 
