The galaxy appears as a centrally concentrated object with a largely smooth morphology, lacking prominent spiral arms or a distinct bar structure. The central region exhibits a bright, yellowish-white hue, indicative of an older stellar population. The galaxy appears nearly circular, suggesting it is being viewed close to face-on. There is a subtle color gradient, transitioning from the warmer, yellowish core to a slightly bluer periphery. No significant signs of ongoing major merger activity or tidal distortions are apparent. The light distribution suggests a spheroidal shape, typical of elliptical or lenticular galaxies.
