The galaxy presents an elliptical morphology, appearing elongated along its major axis. A bright, concentrated nucleus dominates the core region. The light distribution suggests a relatively smooth luminosity profile. The central region exhibits a cyan color, indicating a strong presence of ionized gases, likely from star formation or active galactic nucleus activity. Extending outwards, faint reddish components are visible, potentially representing older stellar populations. The outer regions of the galaxy appear somewhat disturbed, showing possible faint tidal features or minor asymmetries, suggestive of past interactions or mergers. Overall, the galaxy appears to be experiencing, or have recently experienced, some form of disturbance.
