The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. It exhibits a radial color gradient, transitioning from a redder core to bluer outer regions. The galaxy appears elongated, with a high degree of oblateness. There is no discernible evidence of spiral arms or a prominent disk structure. Minor asymmetries or distortions are subtle, suggesting a relatively undisturbed system. Based on the color profile and smooth morphology, this could indicate a galaxy dominated by an older stellar population, with ongoing but low levels of star formation.
