The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge with a yellowish hue, possibly indicating an older stellar population. There is a slight elongation to the galaxy's overall shape. No distinct spiral arms or prominent dust lanes are visible. The lack of pronounced features suggests a relatively quiescent state, with a low rate of star formation. The galaxy is generally round in appearance with no major signs of disturbances due to mergers. The morphology is smooth and featureless, possibly reflecting a galaxy that has undergone significant merging in the past.