The galaxy presents as a relatively smooth, elongated structure, likely an elliptical galaxy viewed at an angle. The central region exhibits a brighter, concentrated glow, indicating a higher density of stars. Moving outward from the center, the light gradually diminishes, suggesting a lower density of stars in the galactic halo. There is little evidence of spiral arms or prominent dust lanes within the galaxy. Its color appears to be somewhat reddish-orange, which could indicate an older stellar population. The galaxy appears largely undisturbed, showing no obvious signs of ongoing mergers or major tidal interactions with other galaxies.
