The galaxy appears as a centrally concentrated, roughly circular object. It exhibits a smooth, featureless morphology with no apparent spiral arms or distinct structures. The light distribution appears to be relatively uniform, with a gradual decrease in intensity from the core outwards. The color profile suggests a bias towards redder wavelengths, with the central regions showing a bluer hue. There is no evidence of significant dust lanes, tidal tails, or other indications of recent major merger events. The overall appearance is consistent with that of an elliptical galaxy or a lenticular galaxy seen face-on, exhibiting characteristics of an evolved stellar population.
