The galaxy presents as a single, relatively smooth object with a cigar-shaped morphology. It exhibits a centrally concentrated brightness profile, suggesting a significant bulge component. Faint disk-like structure may exist but is difficult to resolve, due to the smoothness of the galaxy. There is no apparent evidence of spiral arms or significant dust lanes. Colors appear blended and relatively homogeneous. Hints of blue-green tinges on either end may suggest low levels of star formation but is inconclusive. There is no obvious evidence of a tidal disturbance or merging activity.
