The galaxy presents as a relatively smooth object, with an elliptical morphology. It appears to be quite compact, exhibiting a high degree of central concentration. The galaxy's color suggests a primarily older stellar population, with a hint of a subtle color gradient towards the core becoming more concentrated with older stars. There is little evidence of spiral arm structure or significant dust lanes visible in this observation. There is no obvious signs of any tidal disturbances or ongoing major merger activity. The overall appearance suggests this is likely a mature elliptical galaxy. 
