The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile with no apparent spiral arm structures or distinct dust lanes. The central region displays a high concentration of luminosity, suggesting a prominent galactic nucleus or bulge. The galaxy appears to be slightly elongated, deviating from a perfectly circular shape. There is a subtle color gradient, shifting from a bluer hue in the inner regions to a redder tone in the outer halo, suggesting a change in stellar population with age and metallicity. No major signs of interaction with other galaxies, such as tidal tails or distortions, are readily visible, though a subtle asymmetry cannot be ruled out with the current image resolution. The galaxy appears relatively undisturbed.
