This galaxy exhibits a disturbed morphology, suggestive of a major merger event. The primary body of the galaxy presents a relatively smooth, but asymmetric light distribution, with a brighter, more concentrated central region surrounded by a diffuse, extended halo. There are hints of tidal tails, particularly emanating from either side of the main body, indicating ongoing gravitational interactions. These tails appear faint and somewhat irregular in shape. Overall, the galaxy appears to be actively undergoing a transformation, with a significant portion of its light being emitted from older stellar populations, despite exhibiting some amount of star formation. The overall color index suggests an intermediate composition of stars, with a higher fraction of older stars. The system does not appear to have any clear spiral arm structures or bar features.
