The galaxy presents as an elliptical or lenticular type, with a smooth, diffuse appearance, high central surface brightness, and no obvious spiral arm structure, or bar. It is elongated in shape but tending toward round, without sharp edges or defined features. There is no apparent evidence of dust lanes or significant recent star formation. The galaxy does not appear to be undergoing a major merger or exhibit strong tidal disturbances but may have a minor disturbance based on asymmetry of the light distribution. Its overall morphology suggests it is a relatively quiescent system.
