The galaxy presents as a centrally concentrated, luminous object with an elliptical morphology. The core exhibits a bright, yellowish-white glow, suggesting a significant population of older stars. The light gradually diffuses outward from the core, transitioning to a redder hue in the outer regions. There is no evidence of distinct spiral arms or a well-defined disk structure. The overall appearance is smooth and featureless, suggesting a lack of significant ongoing star formation. A slight elongation is detectable, although the galaxy appears close to circular. No signs of tidal disturbances or interactions with other galaxies are visible.
