The galaxy presents a somewhat smoothed morphology, with a central bulge that appears quite prominent and luminous, exhibiting a yellowish-white hue. There is evidence of a disk-like structure, though it is not sharply defined and shows irregularities. One spiral arm is visible, exhibiting bluer tints indicative of younger stellar populations or active star formation. There may be some minor gravitational disturbances. Overall, the galaxy seems to be in a relatively quiescent state, with moderate star formation activity.
