This galaxy appears to be an elliptical galaxy at a redshift of z = 0.134, indicating significant distance. It presents a smooth, centrally concentrated morphology with no apparent spiral arms or a distinct disk. The galaxy exhibits a generally round shape. There are some indications of very minimal disturbances but the galaxy does not show any signs of major merger activity or interactions. The light is concentrated towards the center, suggesting a dense stellar population likely dominated by older stars. The color profile indicates the galaxy is likely composed of primarily older stars that are not actively forming.
