The galaxy presents as a relatively smooth, elliptical structure. A bright, concentrated core is visible, suggesting a significant concentration of older stars within the galactic nucleus. This central region exhibits a yellowish hue. The galaxy displays a distinct disk-like structure surrounding the core. The outer regions of the galaxy are less defined and somewhat elongated. There is a hint of bluer color within these outer regions. The overall morphology suggests the galaxy has undergone minimal recent major mergers, though there may be some minor gravitational disturbances present, possibly revealed through the slight asymmetry observed in the outer structure.
