The galaxy presents an elliptical morphology with a relatively smooth texture. The galaxy is elongated. The color profile suggests a population of older stars, potentially with a higher concentration of such stars towards the galactic center. There is evidence of a slight disk but this may simply be due to the angle from which we are observing the galaxy. There is no distinct sign of a recent major merger event, though this does not rule out minor disturbances. There is a slight indication of some disruption in the disk but it is hard to ascertain. Overall it is a quiescent galaxy.
