The galaxy presents as a relatively smooth, elliptical-like object. The color profile suggests an evolved stellar population, with a general lack of blue light indicative of ongoing star formation. The redder hue implies a dominance of older, redder stars. There is a very faint hint of some disc-like structure, but is mostly amorphous. No clear spiral arm features or dust lanes are visible, reinforcing the assessment of its smoothed morphology. There is no signs of any ongoing major mergers or other gravitational disturbances. 
