The galaxy presents a somewhat amorphous morphology. The central region exhibits a high degree of luminosity, appearing almost spheroidal. The color gradients suggest the presence of both older stellar populations in the central bulge, indicated by a yellowish-white hue, and younger, bluer stars in the surrounding regions. There's a subtle hint of spiral structure or perhaps just clumpy star formation regions around the central bulge, but it's not a well-defined spiral galaxy. Some degree of disturbance in the outer regions is suggested by the irregular distribution of light. Overall, the galaxy seems to be in a transitional phase, potentially between a spiral and elliptical morphology.
