The galaxy appears to be a relatively compact elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. There is a high degree of circularity observed in the isophotes with a gradual decline in surface brightness moving outward from the core. The galaxy exhibits a dominant bulge component with little to no evidence of a discernible disk or spiral arm structure. The primary color is slightly yellow/white, suggesting an older stellar population with a low rate of ongoing star formation. There are no major disturbances visible in the morphology. The overall shape is well-rounded.