This galaxy appears to be a relatively smooth elliptical, exhibiting high degree of central concentration with diminishing luminosity toward its periphery. The core region displays a yellowish hue, potentially indicative of an older stellar population or dust obscuration. There's little to no visible evidence of spiral arm structures or active star formation regions. The overall round shape suggests a classification tending towards E0-E3 on the Hubble sequence, with minimal apparent flattening. There appears to be no major disturbances or interactions with other galaxies. The galaxy's relatively compact size implies it is at a considerable distance. The light from this galaxy has been redshifted, indicating it is moving away from us at an appreciable fraction of the speed of light. Based on the colors present, the galaxy appears redder and more evolved. Its mass is considerable, placing it among the more massive galaxies. The low star formation rate confirms the galaxy is likely comprised of older stars with less ongoing star formation.