The galaxy appears to be relatively smooth in morphology, with an elliptical-like shape. It does not have any noticeable spiral arms, however, it does exhibit some irregular morphology which could imply a merger is in progress. The main body of the galaxy appears somewhat round but exhibits a slight elongation along one axis. Light distribution across the galaxy appears relatively even, without a strongly defined core. However, the northern portion of the galaxy appears less illuminated. The galaxy shows a slight redder hue relative to the surrounding stars, suggesting older stellar populations, and indicating a lack of recent star formation.
