The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a roughly elliptical morphology, leaning towards roundness, with a bright central bulge. The overall color profile suggests a more evolved stellar population, although some bluer regions are discernible in the outer parts of the galaxy suggesting some on-going star formation. Faint, disturbed morphology can be seen within the outerside of the galaxy. There is faint redder spot at the very bottom of the galaxy which could indicate a region of dust or older stellar population. The galaxy does not exhibit any obvious signs of major mergers or tidal disturbances.
