The galaxy presents as a centrally concentrated, luminous spheroid. The core appears bright yellow, suggesting an older stellar population. A subtle color gradient is observed moving outward from the core, transitioning to more reddish hues in the outer regions. No distinct spiral arms or obvious disk structure are discernible. The galaxy appears relatively smooth and undisturbed, with no signs of major mergers or tidal distortions in the immediate vicinity. The overall morphology suggests a high degree of symmetry and minimal recent star formation in the central bulge and outwards, though redder colors in the periphery may indicate recent or ongoing star formation.
