The galaxy presents as an elliptical morphology, with a smooth light distribution indicative of an early-type system. The central region exhibits a high degree of concentration, characterized by a bright, yellowish core. The outer regions gradually fade in intensity, displaying a redder hue. There are no discernible spiral arms or dust lanes, suggesting a lack of significant ongoing star formation. The overall structure appears largely undisturbed, with minimal evidence of tidal interactions or mergers.
