The galaxy presents as a flattened, elongated structure, suggesting an elliptical morphology with a high degree of ellipticity. Its color gradient transitions from a relatively brighter, yellowish-orange core to a fainter, less defined outer region. The light distribution indicates a smooth profile overall, lacking strong evidence of spiral arms or prominent substructures. There is no obvious nucleus, but a central bulge is possible considering the higher concentration of light in the center. The lack of prominent features suggests a relatively evolved stellar population. The galaxy exhibits no significant signs of ongoing major mergers or tidal disturbances in this image.
