The galaxy appears to be a spiral galaxy viewed at an oblique angle, possibly inclined significantly from our line of sight. The central bulge is prominent and appears relatively smooth and concentrated, exhibiting a yellowish-white color suggesting an older stellar population. Faint spiral arms are visible, though they appear somewhat disrupted, particularly on the lower side of the galaxy. These arms exhibit subtle color variations, with hints of bluer regions indicative of younger, hotter stars. There may be ongoing star formation within the galaxy, particularly in the more disrupted regions.
