The galaxy presents a largely smooth and centrally concentrated morphology. It appears predominantly elliptical, exhibiting a notable degree of roundness, though with a slight deviation towards an intermediate shape. There's no clear indication of significant disturbances or mergers. The galaxy exhibits a subtle color gradient, shifting from a slightly bluer hue in the outermost regions to a redder hue in the central core. Overall the galaxy is estimated to be of considerable mass, and moderate to strong star formation. 
