The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a slight elongation that suggests it may not be perfectly spherical, tending toward a slightly ellipsoidal shape, but it is relatively round. The galaxy's light profile appears to be concentrated in the central region, with a gradual decrease in intensity towards the outer edges, showing no obvious spiral arm structures or prominent disks. There are no obvious signs of major mergers or strong tidal disturbances. Color gradients suggest a possible variation in stellar populations, with a yellow/white core possibly indicating older stellar populations, while hints of bluer colors at the outskirts suggest younger star formation, although this feature is not overly pronounced. Overall, the galaxy presents as a fairly evolved system, likely a massive early-type galaxy undergoing moderate levels of star formation.
