The galaxy presents as a moderate redshift object, appearing as a mildly disturbed system. It exhibits an elliptical shape, with the majority of the light concentrated in a central bulge. While appearing predominantly smooth in structure, there is a subtle suggestion of a disk component, and a hint of minor disturbances in the galaxy's outer regions. There is no evidence of a strong ongoing merger. The color profile of the galaxy suggests an older stellar population, dominated by redder wavelengths.
