The galaxy appears to be an elliptical galaxy. It presents a generally smooth, rounded morphology, exhibiting a high degree of central concentration with the light appearing to gradually fade outward from a bright core. The central region exhibits a yellowish hue, potentially indicating an older stellar population and reduced levels of ongoing star formation. There is no prominent disk structure, spiral arm features, or noticeable dust lanes evident. The overall color profile suggests the presence of evolved stars. The galaxy seems to be undisturbed, displaying no apparent signs of recent mergers or major tidal interactions.
