The galaxy appears to be a luminous elliptical galaxy with a smoothly distributed light profile. It is spheroidal in shape, exhibiting a high degree of roundness. There is no clear evidence of spiral arms or a distinct disk structure. No major distortions or tidal features are observed, which would have been indicative of recent or ongoing major merger activity, although minor disturbances may be present. The galaxy's color indices suggest a population of older stars, with relatively little on-going star formation.
