The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. The core presents a yellow-white hue, suggesting an older stellar population. There is a slight elongation of the galaxy, not perfectly spherical, but approaching a rounded shape. No obvious spiral arm structures or dust lanes are discernible. The red color in some regions indicates the presence of older stars or dust, while the blue light suggests younger populations. Overall, the galaxy seems relatively undisturbed, without evidence of recent major mergers or tidal interactions.
