The galaxy presents as a disturbed system, possibly the result of an ongoing or recent merger. Evident are multiple nuclei, at least three, appearing as bright condensations. There is a distinct tidal feature extending from one side of the galaxy, suggesting gravitational interaction. The color profile varies throughout the galaxy, with some regions exhibiting bluer hues indicative of younger stellar populations, while other areas are redder, suggesting older, more evolved stars. The overall morphology suggests a system undergoing significant dynamic rearrangement. Spiral arm structures may have been present before the disturbance, and the central bulge size does not appear dominant. It is difficult to define whether the galaxy is an edge-on disk, but it exhibits no strong bar feature.
