The galaxy presents as a relatively smooth and concentrated object with an elliptical morphology. It appears to be generally rounded in shape, with a slight elongation noticeable. There is an apparent lack of distinct spiral arms or a well-defined disk structure. The color gradient suggests a higher concentration of older stellar populations. Based on the apparent lack of morphological disturbances, the galaxy appears to be relatively undisturbed. Some possible interaction with minor companions nearby cannot be totally excluded.
