The galaxy appears as a moderately bright, elliptical-like object. Its morphology suggests a relatively smooth structure, with a high degree of central concentration. There is no clear evidence of spiral arms or a prominent disk. The overall color of the galaxy seems to be in the yellow to red range, indicating an older stellar population and a low rate of current star formation. There may be evidence of minor disturbances, and the galaxy could potentially be in the process of merging with another galaxy. However, there is no central nucleus, suggesting that the galaxy's supermassive black hole may not be actively accreting material. The galaxy appears roughly circular in shape.
