The galaxy appears to be a relatively smooth, elliptical system. It is generally round in shape, although there is a slight deviation from perfect circularity. There is some indication of minor tidal disturbances or interactions, potentially hinting at a past or ongoing merger event with a smaller companion. The galaxy displays a centrally concentrated bulge, with light generally becoming more diffuse further from the center. The light profile suggests a relatively old stellar population dominating the bulge. There appears to be a minor amount of ongoing star formation. 
