The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The color profile suggests a dominant population of older stars, with a yellowish hue that indicates relatively low levels of ongoing star formation. There is a slight elongation, but it appears mostly round, exhibiting minimal signs of significant disturbance or recent merger activity, although the image might not fully reveal subtle tidal features. Its structure indicates it is likely a fairly massive galaxy that is relatively quiescent. 
