The galaxy presents as a somewhat disturbed system with hints of a spiral structure, though not particularly well-defined. The central bulge appears bright and slightly elongated, suggesting a possible bar. Spiral arms are suggested by the clumpy, irregular distribution of light emanating from the central region, hinting at on-going star formation within these arms. These regions appear bluer in color, indicative of younger, hotter stellar populations. There are possible signs of a minor disturbance in the galaxy’s morphology.
