The galaxy presents a smooth, elongated morphology. The central region exhibits a bright, concentrated luminosity profile suggestive of a substantial galactic nucleus or bulge. The outer regions display a gradual decrease in brightness, fading into the background. The overall color appears slightly reddish, which could indicate an older stellar population or dust obscuration. No distinct spiral arms or significant star-forming regions are readily apparent. A slight asymmetry in the light distribution might be present, potentially hinting at a past interaction or minor disturbance, though no clear tidal features are visible.
