The galaxy presents as a significantly disturbed system, exhibiting characteristics suggestive of an ongoing or recent merger event. The main galactic body appears elongated and asymmetric, with a brighter, more concentrated core region and an extended, diffuse halo of lower surface brightness. The core region displays a yellowish hue. The outer regions are comparatively redder, potentially indicating an older stellar population, dust obscuration, or ongoing tidal interactions. Evident tidal features are visible, possibly indicating advanced stages of a merging event. The galaxy shows morphological complexity. The overall form deviates significantly from a regular spiral or elliptical structure.
