The galaxy presents as a moderately inclined spiral, exhibiting a disk-like morphology with a central bulge. The bulge appears yellow-white in color, indicating an older stellar population. The disk component shows a mottled blue-ish color suggesting the presence of younger stars and ongoing star formation, though at a low rate. Faint spiral arm structures are hinted at within the disk, though they lack well-defined boundaries. There is evidence of minor disturbances in the overall morphology, possibly indicating a recent interaction or merger event with another galaxy. The galaxy does not have an obvious smooth or elliptical structure, and has a hint of a disturbed structure.
