The galaxy presents as a smooth, elliptical-like structure, exhibiting a dominant bulge. The central region is a bright, concentrated yellow/orange hue, suggesting an older stellar population. Proceeding outward, the colour transitions to a greenish-yellow, implying a lower concentration of older stars, and possibly some ongoing, although relatively low, star formation. The galaxy displays a slight disc-like elongation, deviating from a perfectly spherical shape, with no noticeable spiral arms or major disturbances. The overall light distribution appears relatively uniform and symmetrical. There is no distinct indication of a major merger event, although minor disturbances cannot be ruled out. It is a substantial galaxy, estimated to be ~8.5 kpc across.
