The galaxy presents as a largely smooth, centrally concentrated object. Its overall shape appears elliptical. There is a subtle color gradient visible, with the central region exhibiting a bluer hue compared to the outer regions which seem slightly redder. This hints at a centrally concentrated population of younger, hotter stars and older populations at the outer edges. There is a slight indication of some minor disturbance in the morphology, perhaps an irregularity or faint tidal feature.
