The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a pronounced central bulge that appears bright and yellowish. The outer regions of the galaxy show a subtle flattening, forming a disk-like structure. There is evidence of some star formation, primarily observed along the edges of the disk. A small amount of dust can also be seen from its red emission, although this may also be due to redder stars. The disk component does not display distinct spiral arm structures. Overall, the galaxy appears to be an intermediate stage, possibly between a pure elliptical and a fully developed spiral galaxy.
