The galaxy presents as a spiral structure with tightly wound arms. The nucleus appears bright and yellowish, suggesting an older stellar population. The bulge is moderate in size compared to the disk. The spiral arms display a blueish hue indicating the presence of ongoing star formation. There is a prominent bar structure across the nucleus, with a substantial disk component exhibiting defined spiral arms. The morphology appears relatively undisturbed, with no obvious signs of major merger activity or significant tidal interactions. 
