This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated light profile, with the brightest region located at the core. There is little indication of spiral arm structure or dust lanes; the overall structure is quite uniform. The galaxy exhibits a slightly elongated, though mostly circular shape. The color gradient suggests a population of older stars, possibly with ongoing low-level star formation. There is no evidence of a major ongoing merger, but minor disturbances cannot be ruled out at this resolution. The outer regions fade gradually into the background, with no sharp cut-off observed.
