The galaxy presents a generally smooth, elliptical morphology. A prominent central bulge is visible, exhibiting a yellowish-orange hue, suggesting a significant population of older stars. Surrounding the bulge, a fainter, more diffuse halo extends outwards, displaying a slight flattening. There is a subtle color gradient from the core to the outer regions, with a bluer tint observed in the outer halo, potentially indicating the presence of younger stellar populations, though star formation appears to be low overall. No distinct spiral arms or bar structures are discernible. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or mergers, although there might be minor disturbances present.
