The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color gradient suggests a higher concentration of older stellar populations in the central regions. The outer regions appear slightly bluer, possibly indicating the presence of younger stars, although this is not definitively apparent. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears largely undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. The overall shape is moderately elongated, suggesting an ellipticity that is neither perfectly spherical nor highly flattened.
