The galaxy appears as a centrally concentrated elliptical morphology. It exhibits a smooth light distribution with a fairly symmetrical, rounded shape. There is a slight extension of luminosity which could possibly be indicative of tidal features, indicating possible past interactions. The galaxy's color appears to be on the redder side, suggesting an older stellar population with suppressed star formation. The general form suggests a relaxed system, likely one that has undergone significant morphological quenching. There are two distinct centres of intensity, which, along with the tidal features, may imply this galaxy has been formed by the merger of two seperate galaxies. 
