The galaxy appears as a centrally concentrated object with a smooth, diffuse profile. The core exhibits a bright, yellowish-white hue, which likely indicates a dense population of older stars. This central region gradually fades into a bluer, less luminous halo extending outwards. There is a hint of asymmetry in the outer regions, with a subtle extension or tidal feature visible on one side, suggesting possible past gravitational interactions. The overall shape is predominantly elliptical. While the galaxy's smooth appearance suggests a relatively relaxed morphology, the potential tidal feature hints at minor disturbances. The colour gradient, from yellow-white in the core to bluer in the halo, implies a radial change in stellar populations, with younger, bluer stars more prevalent in the outer regions and older, redder stars dominating the core.
