The observed galaxy presents a somewhat irregular morphology. A faint and diffuse disk is potentially present, though indistinct. There are slight indications of disturbances with a possible minor tidal tail or bridge extending from the galaxy's main body. The galaxy does not appear to be a pure elliptical, there appears to be faint features possibly indicating a spiral nature. The color distribution is not uniform, with subtle variations in the intensity. The galaxy appears to show signs of potential recent or ongoing interaction or merger.
