The galaxy appears as a concentrated, elliptical-like structure. The central region exhibits a yellow-orange hue, suggesting an older stellar population dominating this area. There is a second less luminous central region which may be evidence of a binary or multiple nuclei. The outer regions show some green color which could be evidence of star formation. The galaxy seems relatively smooth and undisturbed, exhibiting little evidence of spiral arms or significant tidal features. It is a moderately luminous galaxy with a red shift indicating that the galaxy is moderately distant. Overall, this galaxy appears to be a relatively massive, evolved system, with signs of recent star formation in it's outer region.
