The galaxy presents as a relatively smooth, centrally concentrated object with a largely spheroidal morphology. There is little evidence of spiral arms or significant disk features. The light distribution appears to be relatively uniform, transitioning smoothly from a bright, yellowish core to a bluer outer halo. Faint irregularities and a hint of a weak feature are potentially visible. There is no obvious sign of a major ongoing merger, though possible minor disturbance or tidal features cannot be ruled out.
