The galaxy presents as a relatively compact, centrally concentrated object. Its morphology appears predominantly smooth, with no obvious spiral arms or bar structure visible. The light distribution suggests an elliptical or lenticular galaxy type. There is a slight elongation and deviation from perfect circularity, but overall, the galaxy's shape is largely rounded. The galaxy exhibits a color gradient, appearing bluer towards the center and redder in the outer regions. There is no evidence of major disturbances or mergers, and any interactions appear minor. The light profile appears to be consistent with an older stellar population.