The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a radial color gradient, transitioning from a yellowish-orange core to a bluer, fainter outer halo. The smoothness and lack of discernible spiral arm structures suggest a lack of active, ongoing major star formation within the disk. The galaxy does not appear significantly disturbed or to be undergoing any major merging events. The overall light distribution is symmetrical, elongated slightly in the horizontal direction. 
