This galaxy exhibits a relatively smooth morphology with a dominant, round central bulge. There is a suggestion of a secondary concentration of luminosity, possibly indicating an ongoing or past interaction or merger. The color profile is generally yellow, suggestive of an older stellar population, although some bluer tinges may indicate regions of more recent star formation. Based on its red color and smooth structure, it is possibly an elliptical or lenticular galaxy at a considerable distance. The overall appearance indicates it is a massive galaxy with a relatively low star formation rate. The luminosity distribution appears relatively concentrated, with light falling off gradually from the core. A close inspection does indicate merging or tidal features.
