The galaxy presents as a luminous, relatively smooth structure with a yellowish hue. It exhibits a centrally concentrated light profile, suggesting the presence of a bulge component, possibly housing a supermassive black hole. Some distortions and diffuse extensions are apparent, indicating potential gravitational interactions or past merger events, in addition to ongoing minor disturbances. These features give it an irregular morphology and a merging aspect, though a portion of the structure appears relatively undisturbed. The overall color suggests an older stellar population, with subdued star formation activity.
