The galaxy exhibits a complex morphology, potentially indicative of an ongoing or recent interaction or merger. The primary body of the galaxy appears elongated and somewhat irregular, with a brighter, more concentrated central region. Emanating from this central area is a distinct tidal tail or stream of material. This tail is relatively long and extended, displaying a diffuse and somewhat clumpy structure, suggesting a history of gravitational disruption.

The overall color of the galaxy is bluish, particularly noticeable in the central region and along the tidal tail. This blueness is suggestive of the presence of younger stellar populations and ongoing star formation. A reddish hue is present within the tail and the disk of the galaxy, which may be indicative of older stars. There are hints of internal structures within the main galactic body, but these features are somewhat blurred. No distinct spiral arms are readily discernible, although there may be the beginnings of a disk-like structure, or a highly disrupted one.
