This galaxy appears to be undergoing a significant interaction or disruption. The primary body of the galaxy presents a relatively smooth and concentrated light profile. The core is bright and somewhat round, suggesting a possible elliptical or lenticular morphology, though the presence of disturbances makes classification challenging.

A prominent tidal tail extends from the main galactic body. This tail is noticeably blue, indicative of active star formation within the stripped material. The tail's morphology suggests a gravitational interaction is responsible for its formation.

Overall, the galaxy's structure is clearly perturbed, deviating from a relaxed spiral or elliptical form. The observed features are consistent with a merger or close encounter with another galaxy, leading to tidal stripping and enhanced star formation.
