Observed galaxy displays a complex morphology, appearing as a non-smooth, featured system with evidence of disk structure. The galaxy presents with a discernible disk, viewed close to face-on. Spiral arm structure appears present but somewhat flocculent and not particularly well-defined. The presence of a central bulge is not particularly prominent. A small amount of light is present from a bulge, but there is likely not a significant bulge overall. There is evidence of ongoing or recent interaction or a major disturbance, with a non-negligible probability of a possible merger event. The overall color index suggests a relatively active star formation rate within the galaxy. The galaxy shape does not present as particularly bar-shaped.
