The galaxy presents a largely smooth and concentrated appearance, suggesting a relatively old stellar population. Its overall shape is elliptical and quite round. The galaxy displays a color gradient, transitioning from a yellowish-white core to a slightly redder outer region. This color suggests a more metal-rich stellar population concentrated in the core, with an older and redder population in the outer regions. There is no evidence of strong spiral arm structure or dust lanes. The galaxy appears undisturbed, showing no obvious signs of recent major mergers.
