The galaxy presents as a somewhat amorphous, centrally concentrated object. The core region exhibits a bright, nearly unresolved appearance, suggesting a high density of stars or possibly an active galactic nucleus. Moving outward from the core, the galaxy displays a more diffuse structure. There is subtle evidence of a very weak disk component, though it is difficult to discern distinct spiral arms or other well-defined features. There may be faint tidal tails or disturbed features hinting at gravitational interactions, or merger events with another galaxy. Further analysis through more detailed imaging and spectroscopic data is necessary to fully understand this system.
