The galaxy appears as a centrally concentrated, luminous object. Its overall color profile exhibits a yellowish core, gradually transitioning into a bluer halo. The central region dominates the light output, suggesting a concentration of older stellar populations. The smoother, more diffuse outer regions hint at a more distributed population of younger, bluer stars. The morphology is predominantly smooth and elliptical, with a high degree of circularity. There are no readily apparent signs of spiral arms or significant disk structures. No major disturbances are visible, though there is a very slight asymmetry in the outer halo, possibly indicating past minor interaction.
