The galaxy presents as a flattened, elliptical structure with a notable tilt relative to the observer. Its light distribution appears smooth, with a gradual decrease in intensity from the center outwards. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a galactic nucleus. The overall color of the galaxy is bluish, which potentially indicates a population of younger, hotter stars, and suggests ongoing or recent star formation activity. There are no clearly defined spiral arms or prominent dust lanes visible in the image. A slight asymmetry is observed, and there appears to be a slight tidal disturbance on one side, suggesting a possible interaction or past merger event.
