The galaxy appears to be elliptical, presenting a relatively smooth, concentrated profile with a noticeable elongation along its major axis. The core region exhibits a bright, concentrated luminosity. Moving outwards from the core, the light intensity gradually decreases. There is evidence of a potential tidal feature on the left side of the galaxy. There are also features on the right side of the galaxy which may indicate a merger event. The color distribution suggests a predominantly older stellar population with a slight reddening in the outer regions. The shape of the galaxy has medium roundness to it.
