The galaxy presents a largely featureless, smooth morphology, appearing predominantly elliptical. The central region exhibits a high concentration of light, diminishing gradually outwards. Color gradients suggest a possible change in stellar population from the core to the outer regions. The overall hue is slightly redder, possibly indicating an older stellar population and lower ongoing star formation. No distinct spiral arms or bar structures are discernible within the resolution of the image. There is a faint indication of some minor disturbance in the outer regions, though no clear signs of ongoing merger activity are observed. The galaxy appears somewhat round in shape.