The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. There is a slight elongation. The color profile suggests a predominantly older stellar population. The galaxy has a high likelihood of not undergoing any major merging events. There is a chance of some minor disturbances in the gravitational field. The central region exhibits a higher concentration of light, indicative of a galactic nucleus. The galaxy is estimated to be of a significant mass. The estimated low star formation rate coupled with its high mass suggest that this is likely a quiescent galaxy.
