The galaxy presents as a centrally concentrated, luminous object. It has a smooth, diffuse appearance, lacking any prominent spiral arms or distinct features typically associated with disk galaxies. The morphology suggests a spheroid-dominated system.

The galaxy's overall shape is mostly rounded, with a slight elongation. There is no readily apparent evidence of ongoing major merging activity or tidal disturbances. The light from the galaxy appears homogenous in color, transitioning from yellow to white at the very center. Given its redshift and apparent magnitude, this galaxy is a fairly luminous object with an estimated mass of over 10^10 solar masses. Its star formation rate appears subdued for a galaxy of its size.
