The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of central concentration. It is primarily bluish-white in color towards the core, suggesting a population of hotter, younger stars concentrated in that region. Fainter, reddish hues are visible in the outer regions of the galaxy, hinting at a population of older, cooler stars. No distinct spiral arm structures or significant dust lanes are discernible. Overall the galaxy has an estimated radius of around 4 kiloparsecs. There are no visual indications of a major ongoing merger, though minor disturbances may be present.
