The galaxy presents as a somewhat amorphous structure, dominated by a central, smooth component. The overall color profile suggests an older stellar population, trending towards redder wavelengths, although there are subtle color variations. The shape is generally elliptical, appearing more rounded. There is some evidence of disturbance in the form of irregularities in the overall structure, indicative of a possible ongoing or recent interaction or merger. It is difficult to tell without further data if the multiple bright sections are areas of concentrated star formation or represent other galaxies being consumed.
