This galaxy appears to be a somewhat elongated, lenticular-type galaxy at a considerable distance, implied by its red-shifted light. It appears to be a red galaxy. It exhibits a relatively smooth light distribution. There is no strong evidence of ongoing star formation or spiral arm structure that is visible in the image. The overall color suggests a stellar population dominated by older, redder stars, indicative of an evolved system. The galaxy is not perfectly circular; it has a cigar shaped morphology, which suggests it may have undergone some type of interaction. There is no visual evidence of strong tidal tails or disturbances.
