This galaxy appears to be a relatively smooth, elliptical system. It has a generally rounded morphology, with a high degree of central concentration. The core is bright and yellowish, indicative of an older stellar population. There is a slight decrease in the brightness from the center to the edge. There are no apparent spiral arms or significant dust lanes, suggesting a lack of current active star formation. The galaxy does not appear to be undergoing any major merging activity, though some minor disturbance cannot be ruled out.
