The galaxy exhibits a generally smooth morphology, with a slight suggestion of a central bulge. Its overall shape is elliptical, appearing mostly round, with a hint of elongation. The galaxy appears to have undergone a possible merging event, with a portion that looks heavily distorted. The light distribution of the galaxy is fairly concentrated, indicating that it is most likely an older galaxy with minimal ongoing star formation. The redder color suggests an older stellar population with lower levels of recent star formation. It is likely a massive galaxy. 
