The galaxy presents a largely elliptical morphology, characterized by a smooth, centrally concentrated light distribution. The core region exhibits a bright, yellowish hue, indicating a higher concentration of older stellar populations. The outer regions appear fainter, with subtle color gradients suggesting some ongoing, albeit subdued, star formation. There is a slight asymmetry to the galaxy's overall shape, potentially indicative of a past minor interaction or internal dynamics. No prominent spiral arms or distinct dust lanes are discernible, further supporting its classification as an elliptical galaxy.
