The galaxy exhibits a spiral structure, presenting as a slightly inclined disk with loosely defined spiral arms. These arms appear somewhat flocculent, showing regions of active star formation distinguished by their bluish tint, especially in the outermost regions of the galaxy. A prominent central bulge dominates the core of the galaxy, displaying a smoother, more concentrated light profile suggesting an older stellar population. The overall morphology is characterized by moderate asymmetry, with some areas appearing more diffuse than others. There are subtle hints of a bar-like structure extending through the central region of the galaxy. The color indices suggest ongoing, though not extremely vigorous, star formation within the disk, while the bulge shows colors consistent with a population of relatively older stars.
