This galaxy appears to be an elliptical galaxy, characterized by a smooth, relatively featureless morphology. It exhibits a high degree of central concentration, with the luminosity decreasing gradually from the core outwards. The galaxy presents a nearly circular shape, showing little evidence of a flattened disk structure. The color profile appears to be dominated by yellowish-red hues, suggesting a population of older stars, with little on-going star formation. There is a faint bluish halo surrounding the core which likely indicates some younger stars. There may be a disturbance caused by a minor merger event happening. Overall, this appears to be a relatively mature galaxy, potentially located at a considerable distance, given the significant redshift associated with it.
