The galaxy presents as a moderately bright, somewhat diffuse object with a dominant central bulge. There is a subtle disk structure, although it is not sharply defined. The galaxy is not perfectly circular; it is somewhat elongated. The overall color is consistent with a relatively older stellar population, with minimal evidence of active star formation regions visible. The galaxy exhibits a smooth texture overall, suggesting it is likely an early-type spiral or lenticular galaxy undergoing a relatively quiescent phase. It may be currently merging with another galaxy. The colors suggest it is at a moderately high redshift.
