The galaxy presents as a relatively smooth, elliptical-like structure with a concentration of light towards the center, indicative of a prominent bulge. There is a gradual decrease in luminosity from the core outwards, suggesting a lack of distinct spiral arms or defined features. The overall color appears to be on the redder side, suggesting an older stellar population and potentially lower ongoing star formation. There is no obvious dust lane or active galactic nucleus visible within the resolution of this image. The galaxy appears to be largely undisturbed, showing no obvious signs of recent major merger activity, though some minor asymmetry cannot be ruled out. The galaxy's shape is somewhat elongated, not perfectly spherical.
