The galaxy presents a disturbed morphology, indicative of an ongoing or recent interaction. The main galactic body appears elongated, with a moderate degree of flattening. There is a prominent tidal tail extending outwards, suggesting gravitational disruption. Within the central region, there is a complex distribution of light, with a brighter core exhibiting evidence of active star formation, potentially triggered by the interaction. Overall, the galaxy's structure appears asymmetrical, with a significant deviation from a regular spiral or elliptical form. Dust lanes are subtly apparent, particularly in the brighter, central regions.
