The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. The light profile suggests a dominant bulge component. The color is predominantly yellow-orange, indicative of an older stellar population with fewer young, blue stars. There is little evidence of spiral arm structure or significant dust lanes. The overall morphology suggests a galaxy that has largely ceased significant star formation activity. There are no obvious signs of tidal disturbances or ongoing mergers. The galaxy appears isolated and undisturbed.
