The galaxy exhibits a disturbed morphology, characterized by a prominent tidal tail or bridge extending from the main galactic body. The primary galactic component displays a somewhat amorphous shape, hinting at potential ongoing interactions or recent merger activity. A distinct, compact structure is observed near the primary body and exhibits a different color profile which indicates differing stellar populations or composition. Overall the system presents as a complex, likely interacting, configuration. Star formation appears to be localized in the main body with an actively forming population of stars.
