The observed galaxy presents a complex morphology indicative of an ongoing or recent merger event. A prominent spiral structure is disrupted, exhibiting loosely wound arms. Two of these arms are clearly discernable. The central bulge appears moderately sized and diffuse. Evidence suggests the presence of a bar feature. The main galactic body is not edge-on. Areas of active star formation, characterized by bluish hues, are interspersed within the spiral arms. Tidal tails and other signs of gravitational interaction are apparent. There appears to be 4 or more distinct objects involved in the interaction.
