The galaxy exhibits an elliptical morphology with a moderate ellipticity, appearing somewhat elongated rather than perfectly spherical. The central region displays a smooth, featureless light distribution, characteristic of an older stellar population. The light emitted from the central region is primarily redder in color, suggesting a dominance of evolved stars. There appears to be a feature or disturbance near the bottom of the image. The blue color might indicate the presence of some ongoing star formation, however the merging classification indicated a 23% chance of an on-going major merger which could affect the morphology and color of this region. The galaxy appears to be relatively massive, with an absolute magnitude indicating a luminous object at its redshift. The low star formation rate relative to its mass implies a quiescent or passive galaxy with minimal current star formation activity in much of the galaxy, with the possible exception of the area mentioned above.
