The galaxy presents a generally smooth, elliptical morphology. Its light is dominated by a reddish-yellow hue, suggesting a population of older stars and relatively low ongoing star formation. There appears to be a merging occuring, with a primary central mass and a few distinct clumps of luminosity scattered around it that are not entirely indistinct, and some light connecting them. The luminosity and mass estimates would indicate this is a fairly large galaxy. The round morphology, dominant redder colors, suggest it is most likely a fairly old galaxy. The merging is not perfectly distinct, suggesting it may have been taking place over a long duration. 
