The galaxy presents as an elliptical or lenticular type. It has a centrally concentrated, smooth and bright bulge, decreasing in luminosity outwards, with a fainter surrounding disk or halo. The galaxy exhibits a generally round morphology, with no clear spiral arm structures visible. There is some evidence of a slight asymmetry or minor disturbance in the outer regions, though no major merger event is apparent. Color gradients within the galaxy indicate a possible variation in stellar populations, with the central bulge appearing yellower and more red than the outer regions, which may indicate ongoing star formation.
