The galaxy presents a predominantly smooth morphology, exhibiting a high degree of central concentration. It appears largely elliptical or spheroidal in shape, with a high degree of roundness and minimal visual distortions. The galaxy displays a subtle color gradient, with a slightly reddish core transitioning to a bluer outer halo, potentially indicating variations in stellar population ages, a population of older stars towards its core, and a presence of relatively young stars in the halo. The red shift indicates this galaxy is at a substantial distance. No spiral arm structures or significant tidal features are discernible. The general morphology suggests that the galaxy may be relatively evolved, experiencing low levels of star formation activity. There is some minor disturbance in the structure, which could be evidence of a recent, small merger.
