The galaxy appears as a luminous, elliptical structure, elongated along its major axis. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or distinct dust lanes. The central region displays a high surface brightness, indicating a concentrated stellar population or an active galactic nucleus. The color gradient suggests a redder core, potentially indicative of an older stellar population or dust obscuration, transitioning to slightly bluer hues in the outer regions, possibly due to ongoing star formation. The absence of significant tidal features suggests it is not currently undergoing a major merger event, although a minor disturbance cannot be ruled out given the subtle asymmetry in its outer isophotes. The galaxy's overall structure indicates it is likely an evolved system, potentially a lenticular or elliptical galaxy, located at a considerable distance from our own.
