The galaxy presents as a relatively compact, elliptical morphology. Its light distribution appears smooth and centrally concentrated, lacking any prominent spiral arm structures or distinct features indicative of active star formation. The observed color suggests a population of older stars, potentially indicative of a passively evolving system. The overall shape appears more rounded than elongated, with no visible tidal features or signs of recent mergers or major disturbances, although there is a potential companion galaxy or foreground object in the upper portion of the image that may be influencing the overall structure of the target galaxy.
