The galaxy appears to be relatively smooth and elliptical in shape, lacking a prominent disk or spiral arm structure. The light distribution suggests a centrally concentrated bulge. The galaxy exhibits a yellowish-red hue, indicating an older stellar population with relatively low ongoing star formation. It may be in the process of merging with another galaxy or may have completed a merger in the past, as it appears slightly disturbed with a few prominent clumps of brighter light within the galaxy. The galaxy is compact.