The galaxy presents a spiral morphology, observed at a relatively face-on orientation. A distinct central bulge is visible, with a yellow-white hue, indicating a concentration of older stellar populations. The spiral arms are prominent and loosely wound, displaying a blue tint that suggests ongoing star formation. The galaxy shows signs of a possible bar structure in the inner regions. The galaxy's disk is not perfectly symmetrical, exhibiting some subtle distortions that could be indicative of minor gravitational interactions.
