The galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of central concentration. It exhibits a bright, yellowish core, suggesting an older stellar population. The light gradually diffuses outwards from the core into a fainter, more indistinct halo. Some bluer regions can be distinguished in the halo, possibly indicating areas of ongoing, though not particularly vigorous, star formation. There are suggestions of some minor disturbances in the outer parts of the galaxy, but it doesn't seem to be significantly interacting with any other galaxy. The overall structure indicates that it is likely a massive galaxy.
