This galaxy exhibits a somewhat elliptical morphology, appearing largely smooth and concentrated. The light is more concentrated centrally and the outskirts fade in intensity. There's evidence of asymmetry or tidal disruption to one side of the galaxy. One distinct redder region is visible, that may be the product of a merger event. There appears to be a higher concentration of older stellar populations in the smoother body of the galaxy, giving it a yellowish hue. The redder structure appears to be significantly disturbed, possibly indicating it is an infalling structure. There is little evidence of ongoing, large-scale star formation across the primary body of the galaxy; it appears to be a relatively quiescent system overall.
