The galaxy presents as a primarily smooth, elliptical-like system. The central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars. Surrounding the core, there's a fainter, more diffuse halo of light, extending outwards with a subtle, almost imperceptible disk component. There's evidence of minor disturbances in the overall symmetry, though they do not strongly suggest a recent major merger. The galaxy appears yellowish-orange, which could imply an older stellar population. Faint blue tinges within the halo region hint at the presence of some younger stars or regions of active star formation, albeit at a low rate.
