The galaxy presents a morphology suggesting a transition from a smooth elliptical form to a more structured disk-like system. The central bulge exhibits a pronounced concentration of light, appearing yellowish-white, indicative of an older stellar population. Surrounding this bulge is a fainter, bluer halo with hints of spiral arm structures. The galaxy shows some visual asymmetry, possibly suggestive of minor gravitational interactions or internal disturbances. Overall the galaxy has a significant mass with some star formation occuring.
