The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a high degree of central concentration, with a bright, luminous core that fades gradually into the surrounding galactic halo. The core appears to be comprised of older stellar populations, indicated by the yellow-white color. The outer regions demonstrate some irregularities and faint spiral arm-like features, though the overall structure leans towards smooth. There are likely signs of minor disturbances in the morphology. Overall the galaxy has a relatively low rate of star formation.
