The galaxy appears to be a relatively smooth, elliptical structure. Its morphology is dominated by a centrally concentrated bulge with a radial decrease in surface brightness. There is a slight elongation, deviating from a perfectly circular shape. There is a hint of a disk structure but not enough to call it a spiral galaxy. The galaxy has a yellow hue, suggesting an older stellar population with minimal ongoing star formation. There is no evidence of any major merging events, though there are subtle signs of minor disturbances. The galaxy appears to be moderately massive.