The galaxy presents as a luminous, elongated structure. The central region exhibits a high concentration of light, appearing as a bright, unresolved core. Surrounding the core, the light gradually decreases outwards, forming an extended, diffuse halo. The overall color appears to be relatively uniform with slight variations in hue, possibly indicating subtle differences in stellar populations across the galaxy. The galaxy appears to be relatively smooth and does not show strong evidence of spiral arms or other distinct features. The morphology suggests this may be an elliptical galaxy, possibly of type E4-E6, based on its ellipticity. There is a slight hint of asymmetry, particularly along the major axis, which may indicate minor disturbances or interactions, although a clear merging event is not apparent.
