The galaxy presents as a somewhat elliptical system, with a notably brighter central region suggestive of a substantial galactic nucleus. The overall colour profile appears slightly blue-shifted, indicating the presence of younger stellar populations or ongoing star formation. There is some evidence of disrupted morphology or faint tidal features surrounding the primary galactic body, possibly indicating an interaction or recent merger event with a smaller system. The galaxy's moderate angular size suggests it is not a particularly nearby system, and that the bright central region could potentially be concealing an active galactic nucleus.
