The galaxy presents as an elliptical morphology with a high degree of central concentration. The core exhibits a bright, luminous glow, indicative of a dense stellar population. Moving outward from the core, the light gradually fades, forming a diffuse halo. The galaxy displays a notable degree of flattening; its shape is oval rather than perfectly circular. There's a subtle color gradient, transitioning from a yellowish-white core to a more bluish outer region. No distinct spiral arm structures or dust lanes are visible. The smooth light distribution suggests that star formation is either minimal or absent.
