The galaxy appears to be a luminous, centrally concentrated system. Its overall morphology suggests it is likely an elliptical galaxy or a lenticular galaxy viewed close to face-on, exhibiting a smooth and featureless light distribution. The galaxy has a generally round shape with a slight elongation, but no apparent spiral arms or distinct structures. A bright, almost stellar-like core is visible, surrounded by a more diffuse halo of light. The galaxy appears to be relatively isolated, showing no signs of significant tidal interactions or major mergers, although there may be minor disturbances present. The color gradient implies a stellar population that is somewhat bluer in the outer regions compared to the very center. The estimated size is approximately 6 kpc in diameter. The blue color observed may indicate ongoing star formation. The redshift indicates that the galaxy is at a considerable distance.
