The galaxy presents a generally smooth and somewhat elliptical morphology. The central region exhibits a higher concentration of light, appearing bright and yellowish-white, suggesting a population of older stars. There appears to be very little or no observable spiral structure and there are no signs of a large, significant galactic bar. There are faint hints of bluer light, possibly indicative of some active star formation, concentrated towards one end of the galaxy. Some indication exists of a minor merger or disturbance to the morphology of the galaxy on the other end. Overall, the galaxy appears to be a relatively quiescent system.
