The galaxy presents a generally elliptical morphology, appearing somewhat flattened. The central region exhibits a high surface brightness, with a concentration of light. Progressing outwards from the core, the light gradually diminishes. There are no distinct spiral arms, bar structures, or dust lanes visible. The color profile suggests a relatively uniform stellar population, with a slight bluish hue suggesting some recent star formation, especially in the central regions. No prominent features indicative of active galactic nuclei activity, such as jets or strong emission lines, are observed in the image. The overall structure is relatively smooth and undisturbed, lacking any signs of major ongoing merger events.
