The galaxy presents as a largely smooth, elliptical structure. The central region exhibits a bright, concentrated core that diffuses outwards. The light profile appears to be relatively uniform, lacking prominent spiral arms or distinct morphological features. The overall shape is approximately round, with only minor deviations from perfect circularity. There is little evidence of ongoing or recent major merger activity or significant tidal disturbances. Color gradients suggest a redder central population, possibly indicating an older stellar population and reduced star formation activity within the core region. The faint outer regions are bluer, which might mean some star formation is happening, or just that there are younger stars there.
