The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, exhibiting a high degree of roundness. A slight color gradient is discernible, transitioning from a more yellowish-white core to a subtly redder outer region. There is little evidence of distinct spiral arms or a prominent disk structure. The overall light distribution suggests an evolved stellar population, potentially indicative of a relatively low star formation rate. No significant signs of ongoing mergers or major disturbances are apparent in the image. The galaxy presents a uniformly featureless texture.
