The galaxy exhibits a generally smooth, elliptical morphology. The central bulge appears bright and concentrated, with a yellowish-white hue, suggesting an older stellar population. The galaxy appears slightly elongated, showing a minor axis about 70% of the length of the major axis. There is very little in the way of apparent spiral arm structure or dust lanes within the observable morphology. A faint disk is implied by the flattened shape, but it is quite featureless. The overall color profile suggests a relatively passive galaxy with minimal ongoing star formation. There are no indications of tidal tails, shells, or other significant morphological disturbances indicating a recent major merger event.
