The galaxy presents as a spiral, viewed at a moderate inclination, not quite edge-on. A bar-like structure is visible across the central bulge region, exhibiting hints of a strong component. Faint, loosely wound spiral arms extend from the bar and central bulge, these are patchy in appearance. The central bulge appears moderate in size, exhibiting a yellow-white hue, possibly indicating an older stellar population. The spiral arms show a bluer coloration, suggesting the presence of ongoing star formation. There are no visible signs of any major merger events or significant tidal disturbances. The galaxy shows disk-like characteristics.
