The galaxy appears as a single, relatively smooth object, potentially an elliptical galaxy or a lenticular galaxy viewed at an angle. It displays a central concentration of light that gradually fades towards the outer edges. The core region exhibits a bluish-white hue, indicative of some amount of younger star formation or a population of hotter, bluer stars. There's a slight elongation to the overall shape, suggesting it isn't perfectly spherical. No prominent spiral arms or dust lanes are visible in this observation. There seems to be no evidence of major ongoing mergers or significant tidal disturbances.
