The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its color is generally yellowish, which may indicate an older stellar population. There is a suggestion of a slightly flattened shape, but it appears mostly round, with no obvious spiral arm structures or significant dust lanes visible. The outer regions of the galaxy fade gradually into the background sky, with no sharp edges. There is no clear evidence of a recent or ongoing major merger event, although some very minor disturbance cannot be ruled out.
