The galaxy presents a generally smooth appearance with a high degree of central concentration. It exhibits an elliptical shape with a dominant spheroidal component. The color profile suggests a bulge region dominated by older stellar populations, appearing yellowish-orange. There appears to be a faint disk feature. There are no readily apparent spiral arms. The overall structure suggests a classification towards the early-type end of the Hubble sequence. There appears to be a slight disturbance to the shape of the galaxy, especially on the left side. This could be due to a merger of some kind with another galaxy.
