The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light is centrally concentrated, with a radial falloff from the central region. The galaxy appears largely elliptical, with a high degree of roundness. There are some irregular features to the surrounding area of the central region, which appear to be tidal arms or streams caused by minor disturbances of a merger event. There is no evidence of a significant disk component or spiral arm structure. It is possible this galaxy is in the late stages of a minor merger. Overall, the galaxy appears relatively isolated and undisturbed, aside from the potential signs of a minor merger.
