The galaxy presents a largely smooth morphology, with a high degree of central concentration. Its shape approximates a rounded form. There is very little indication of spiral arm structure or significant disk features. The central region is luminous, with a colour index suggesting a population of older stars. The outer regions appear fainter, gradually decreasing in intensity away from the core. There may be a very slight distortion or minor disturbance present, although the overall structure appears relatively undisturbed. The galaxy does not obviously appear to be undergoing a major merger.
