The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, with a shape between round and cigar-shaped. A bulge is visible, exhibiting a yellowish hue. The galaxy shows no strong evidence of spiral arm structure or prominent dust lanes. There are no indications of tidal tails, major distortions, or ongoing mergers. There may be slight disturbances that are very minor within the galaxy. The galaxy appears to be a fairly isolated system in a relatively advanced stage of evolution.
