The galaxy exhibits a morphology that is neither purely elliptical nor purely spiral, but presents characteristics of both. The central region is dominated by a smooth, concentrated bulge, exhibiting a yellowish-orange hue suggesting an older stellar population. Extending outwards, there is evidence of a disk-like structure, though it appears disturbed or irregular. One side of the disk shows a bluish tint indicative of younger, hotter stars, possibly regions of ongoing star formation. The opposite side appears more diffuse and less defined. There's a hint of tidal distortion, which can be caused by the gravitational interaction of galaxies. The structure and color distribution suggest the possibility of a recent or ongoing merger event.
