The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a generally rounded morphology, lacking prominent spiral arms or a well-defined disk. The light profile is relatively smooth and symmetric. There is some indication of minor disturbances or faint tidal features extending from the galaxy's core. The color appears to be somewhat redder, which suggests an older stellar population and a lower rate of ongoing star formation within the galaxy. There is no evidence of a recent major merger or significant interaction with another galaxy.
