The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting an elliptical morphology. There is a clear radial gradient in brightness, with a bright, compact core that diffuses outwards into a more extended, fainter halo. The overall color profile suggests an older stellar population, possibly with reduced ongoing star formation. It is characterized by an apparent lack of spiral arms or prominent dust lanes, contributing to its smooth appearance. Based on these observations, it can be identified as a galaxy, likely an elliptical galaxy, located at cosmological distance. It does not appear to show any signs of active galactic nuclei or any interactions with another galaxy nearby.
