The galaxy presents an elliptical morphology with a dominant, smooth central bulge. The light distribution appears centrally concentrated, fading gradually outwards. The isophotes exhibit a degree of ellipticity, suggesting a flattened spheroidal shape. The color gradient transitions from a yellowish-white core to a bluer hue in the outer regions, potentially indicating younger stellar populations present in the disk. No distinct spiral arm structure is apparent. The overall appearance suggests a system with a moderate degree of internal organization, consistent with a galaxy undergoing steady star formation. There is no major disturbance to the morphology, ruling out the possibility of a major merger.
