This galaxy presents as a generally smooth, centrally concentrated object with a roughly elliptical morphology. The core exhibits a bright, yellowish-white glow. The light appears to diminish gradually from the center outwards to the edges. There is little to no visible spiral structure or obvious dust lanes present. The overall color suggests an older stellar population. A slight irregularity or extension is suspected on the lower edge of the galaxy. There are no signs of a major ongoing merger, but the possibility of minor tidal disturbances cannot be completely ruled out.
