The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated luminosity, decreasing in intensity towards the outer edges. There is a slight elongation and is mostly round. The color appears yellow, suggesting an older stellar population and a reduced rate of star formation. No significant dust lanes or spiral arm structures are readily apparent. There is no indication of a major merger. It may be undergoing a minor disturbance. The overall appearance suggests a mature system that is not actively forming stars at a high rate.
