The galaxy presents as a relatively smooth, elliptical-like structure. The primary body of the galaxy exhibits a concentrated, centrally located bulge. There is some evidence of tidal disturbances, most notable a second bright region above and to the right of the main bulge of the galaxy. There also seems to be some light suggesting there could be another disturbance below and to the left of the bulge. The color gradient suggests a possible mix of stellar populations, transitioning from bluer hues in the fainter outer regions to a redder core, indicative of older stars. The overall morphology suggests a system that has potentially undergone at least one past merger event and may be currently undergoing another.
