The galaxy appears to be elliptical in morphology, with a smooth, centrally concentrated light distribution. The galaxy exhibits a fairly high degree of roundness. There is evidence of a possible merger event or tidal interaction. This is revealed by a secondary condensation that is near the primary mass of the galaxy. The color index implies the galaxy's stellar population is dominated by older, redder stars, suggesting a relatively quiescent, evolved system. There does appear to be some asymmetry present, which could possibly be a feature in the galaxy. Overall, this galaxy could potentially be in a merging process. 
