The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile is centrally concentrated, exhibiting a bright, dense core that gradually diffuses outwards. There is a slight elongation, suggesting it is not perfectly spherical. The galaxy displays a color gradient; the central region appears more yellow/white, possibly indicating an older stellar population, while the outer regions show a subtle hint of bluer hues, implying some ongoing or recent star formation. There is no obvious spiral arm structure or dust lane features. The galaxy appears relatively undisturbed with no signs of recent major mergers.
