The galaxy presents as a fairly smooth, elliptical-shaped structure. Its core exhibits a concentrated, bright yellowish-white light, suggesting a significant population of older stars. Moving outwards from the core, the light gradually diffuses, transitioning to a less intense, more reddish hue in the outer regions of the galaxy. There is no apparent disk structure or spiral arm morphology visible. The overall appearance indicates minimal ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of a major merger event or significant tidal distortions. The axial ratio suggests a moderate degree of ellipticity, as opposed to being perfectly spherical.
