The galaxy appears as an elliptical-shaped object, displaying a smooth, featureless morphology without any apparent spiral arm structures or dust lanes. The color profile indicates a dominant yellow-orange hue, suggesting a population of older stars and a low rate of current star formation. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer edges. There are no signs of ongoing major mergers or significant tidal disturbances. The galaxy exhibits a moderate redshift, indicating that it resides at a considerable distance. Given the observed characteristics, this object is likely an elliptical galaxy dominated by an evolved stellar population.
