The galaxy presents with a complex morphology, appearing to be in a late stage of interaction or exhibiting significant internal disturbances. The central region is somewhat indistinct, with a diffuse light profile, making it difficult to classify a precise nuclear structure.

A prominent feature is the asymmetrical distribution of light, particularly evident in the lower section of the galaxy. The presence of tidal tails or streams are strongly indicated. The colors are strongly suggestive of active star formation within these tidal features.

Overall, this object displays characteristics indicating a non-equilibrium state, with a complex interplay of gravitational forces likely driving its current morphology. Further spectroscopic analysis would be beneficial in determining the nature of the interactions, star formation rates, and the overall composition of this system.
