This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a generally round morphology, with no obvious spiral arm structures or bar features visible. The light distribution suggests a concentration of older stars toward the center, indicated by a yellowish hue in the core. The outer regions appear bluer, possibly indicating the presence of a younger stellar population or some ongoing, though limited, star formation. There is no readily apparent dust lane or significant signs of recent or ongoing merger activity. The galaxy displays a relatively uniform surface brightness profile, with a gradual decline in luminosity from the core outwards. 
