The galaxy presents as a relatively compact object with a smooth, centrally concentrated light profile. It exhibits an elliptical or lenticular morphology, showing minimal evidence of spiral arms or a distinct disk structure. Its shape appears nearly round. The galaxy is approximately 8 kpc in radius. Its estimated distance from Earth places it at a significant redshift. There appears to be no major or minor disturbances due to mergers.

The galaxy's color indices suggest the presence of a moderate stellar population. Based on the image, star formation activity seems minimal.
