The galaxy presents as a relatively smooth, elliptical morphology. The light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions, suggesting minimal presence of distinct features such as spiral arms or a prominent disk. The galaxy exhibits a yellowish-white hue at its core, potentially indicative of an older stellar population dominating the central region, with slight variations in color towards the outer regions that indicate the presense of younger stars. Overall, there is no indication of ongoing major mergers or significant tidal disturbances visible in the image. The structure appears largely undisturbed and consistent with a quiescent galaxy.
