The galaxy presents a generally smooth morphology with a bright central bulge. The light distribution appears to be centrally concentrated, fading gradually outwards. The galaxy shape appears more elliptical than disk-like, with the observed ellipticity being moderate. There is no strong evidence of spiral arm structure or significant dust lanes. Hints of some faint outer structure can be seen, which is not perfectly symmetrical and slightly disturbed in shape. The overall appearance indicates a relatively evolved system. No major merger event appears to be occurring, but there is a slight chance of a minor merging interaction or minor tidal disturbance. The central region is significantly brighter than the outer regions.
