This galaxy presents as an elliptical or lenticular system. It appears largely smooth in texture with a dominant central bulge. The color gradient transitions from a yellow-white core to a slightly bluer outer halo, hinting at a differential stellar population distribution with potentially older stars concentrated centrally. The overall shape is moderately elongated, showing a deviation from perfect circularity. There is no clear evidence of significant spiral arm structure, major disturbances, or ongoing mergers within the visible light bands.
