This galaxy exhibits a disturbed morphology, characterized by a prominent tidal tail extending outwards from the main galactic body. The central region appears relatively smooth and concentrated, with a color profile that suggests an older stellar population. The tidal tail is noticeably bluer, indicating the presence of younger stars and ongoing star formation. The galaxy's disk is likely inclined to our line of sight, possibly nearing edge-on. There is evidence of significant gravitational interaction, perhaps due to a recent or ongoing merger event with another galaxy. The system displays signs of active star formation within the tidal features, implying a dynamically disturbed environment where gas is being compressed and triggering stellar birth.
