The galaxy presents as a single, generally smooth structure, exhibiting an elliptical morphology. The light distribution suggests a high degree of central concentration, with luminosity decreasing gradually from the core. The galaxy appears to be relatively featureless; there is no readily apparent spiral arm structure or dust lane obscuration. Color gradients show a distinct shift from a bluer central region to redder outer regions, possibly indicating differences in stellar population age and metallicity. There are no signs of major mergers or tidal disturbances in the image. The overall appearance suggests a relatively evolved system.