The galaxy appears to be an elliptical galaxy at intermediate redshift. It exhibits a largely smooth morphology, with no readily apparent spiral arms or a distinct disk structure. The light distribution is centrally concentrated, with a bright core that gradually decreases in intensity outwards. The overall shape is approximately elliptical, tending slightly towards an "in between" shape with only a very small chance it is cigar-shaped. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although minor disturbances cannot be ruled out. The color indices suggest a population of older stars dominating the stellar content. The galaxy is of substantial mass and exhibits a relatively low star formation rate.
