The galaxy appears to be a relatively smooth and centrally concentrated object. It exhibits a generally elliptical morphology, with a high degree of roundness. There is no readily apparent disk structure or spiral arm features visible. The color profile suggests a population of older stars, with a redder overall hue. There is no obvious evidence of ongoing major mergers or significant tidal disturbances, though subtle minor disturbances may be present. Given the apparent size and smoothness, this galaxy is likely a massive elliptical galaxy, observed at a redshift placing it at a considerable cosmological distance.
