This galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core is a bright, yellowish hue, possibly indicating an older stellar population dominated by red giant stars. The light gradually diffuses outward from the core, creating a halo effect. There are subtle color gradients within the galaxy, transitioning from yellow in the core to slightly redder tones in the outer regions. No distinct spiral arm structures or dust lanes are visible. The galaxy appears generally undisturbed, showing no signs of major mergers or tidal interactions. Its overall morphology suggests a well-relaxed system.