The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a subtle elongation, appearing more "in between" round and cigar-shaped than either extreme. There is an apparent lack of significant spiral arm structure or prominent dust lanes. The central bulge is prominent and appears to be relatively old stellar population based on the yellowish orange color, potentially indicating less active star formation. The galaxy does not display obvious signs of a major ongoing merger, though a potential minor disturbance or interaction cannot be ruled out from this image alone. Overall, the galaxy seems to be a mature, fairly quiescent system with a high degree of central concentration.
