The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentration of light towards the center. There is a slight elongation visible, with an axis ratio appearing close to unity. No prominent spiral arms or distinct features are discernible. There appear to be some faint irregularities in the outer regions. The galaxy appears to be relatively isolated, with no obvious signs of a major merger. The galaxy's color index suggests it may be older, with lower ongoing star formation.
