The galaxy presents as a primarily smooth and elongated object, likely an elliptical galaxy, seen at an oblique angle relative to our line of sight. Its central region exhibits a concentrated brightness, suggesting a dense core of stars. Moving outward from the center, the light gradually diminishes, fading into the surrounding space with a diffuse halo. There is a subtle color gradient; the core appears slightly more yellowish, potentially indicating an older stellar population, while the outer regions show hints of bluer hues, suggesting the presence of some younger, hotter stars. Overall, the galaxy's structure is relatively undisturbed, displaying no prominent spiral arms or other significant features, although there is minor asymmetry.
