This galaxy appears to be a relatively smooth, centrally concentrated object. The light distribution suggests an elliptical morphology. There's a dominant, bright core, likely indicating a high concentration of stars. The color gradient transitions from a yellowish-white central region, indicative of older stellar populations, to a slightly bluer outer halo. This suggests that the galaxy may have experienced a minor star formation event in the more recent past, albeit not to a substantial degree. The overall roundness indicates it does not have a distinct disk or spiral arm structure. There are no obvious signs of major tidal disturbances or ongoing mergers.
