The galaxy appears as a luminous, elliptical object with a smooth, featureless morphology. It exhibits a color gradient, transitioning from a yellowish-white core to a slightly redder halo. The shape is elongated, suggesting a potential oblate spheroid structure. There is no apparent spiral arm structure or dust lane obscuration visible in this image. The absence of distinct features and the smooth color distribution suggests a relatively quiescent stellar population with low ongoing star formation. The galaxy appears relatively isolated with no strong indications of a recent or ongoing merger event. The spatial extent of the galaxy is moderately large.
