The galaxy presents a distinct spiral structure, exhibiting prominent spiral arms. Two primary arms appear to emanate from the central bulge region, winding loosely outwards. Star formation regions are suggested by the irregular distribution of light and color along the arms. The central bulge appears moderate in size and exhibits a yellowish hue, potentially indicating an older stellar population. The overall color of the galaxy leans towards the redder end of the spectrum, suggesting a possible redshift and significant distance. There is no obvious evidence of a strong bar structure. The galaxy shows some signs of disturbance, although not necessarily a recent major merger.