The galaxy presents a predominantly smooth morphology, with a relatively high degree of central concentration. Its shape appears to be neither perfectly spherical nor highly elongated, but rather an intermediate form. There is a subtle suggestion of a disk-like structure, although the smoothness of the overall light distribution predominates. Faint hints of disturbed features are visible, such as what appear to be tidal tails. The color gradient transitions from a yellowish hue at the core to a bluer tinge in the outer regions, possibly indicative of differing stellar populations. Overall, the galaxy is considered to be relatively massive, with a moderate rate of star formation.
