The galaxy presents as a spiral with a prominent disk structure. Spiral arms are clearly visible, exhibiting a somewhat patchy distribution of light, suggesting active regions of star formation along their lengths. The arms appear grand design with a flocculent substructure. The bulge is moderate in size, contributing a significant fraction to the overall light profile of the galaxy. The bulge color is noticeably yellower compared to the disk, implying an older stellar population. There is no strong evidence of a bar structure. The disk of the galaxy is not seen edge-on, and there is no obvious sign of any ongoing major merging events or significant tidal disturbances.
