The observed galaxy presents an overall elliptical morphology. The light distribution appears relatively smooth and concentrated towards the center. The core exhibits a bright, almost unresolved appearance, indicative of a high stellar density. Moving outward from the central region, the light gradually decreases with no distinct features such as spiral arms or a prominent disk visible. The color gradient seems to be subtly redder towards the center and bluer in the outer regions, which suggests potential differences in stellar populations and/or dust content across the galaxy. Overall, the galaxy's structure is mostly undisturbed, with no obvious signs of recent major mergers or significant tidal interactions.
