The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. Its shape is predominantly round, with a slight elongation that deviates minimally from perfect circularity. The galaxy demonstrates a color gradient, with the central region appearing a yellowish-white, suggestive of an older stellar population and potentially dust obscuration. Moving outwards from the center, the color shifts toward a slightly bluer hue, indicating the presence of a younger stellar population. There is no readily apparent spiral structure or distinct arms; rather, it appears as an elliptical or lenticular galaxy. No signs of major mergers or significant tidal disturbances are discernible.
