The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a predominantly spheroidal morphology, potentially an elliptical galaxy or a lenticular galaxy seen face-on. There is a subtle color gradient, with the central region appearing more yellow/gold, possibly indicating an older stellar population. Fainter, bluer light is observed in the outer regions of the galaxy, which may be caused by a younger, less centrally concentrated stellar population. The overall form lacks any obvious spiral arms or strong morphological features indicative of recent major mergers. A high degree of rotational symmetry is apparent. The galaxy appears to be isolated, with no visible signs of tidal interactions or nearby companion galaxies that would imply ongoing merger activity. The overall appearance is consistent with a galaxy that has largely ceased significant star formation in its core, while outer regions may be in a transition stage.
