The galaxy presents as a single, relatively smooth object, exhibiting a generally elliptical morphology. It shows a high degree of central concentration, with luminosity decreasing gradually from the core outwards. There is no apparent spiral arm structure or distinct disk component visible in this image, suggesting this may be an early-type galaxy. The galaxy is generally round, although there is a hint of deviation. There does not appear to be any signs of recent or ongoing major merger activity or significant tidal disturbances, it appears to be a relatively undisturbed system.
