The galaxy appears as a single, moderately concentrated object. Its light is predominantly in the redder wavelengths, suggesting an older stellar population and/or significant dust obscuration. There are subtle indications of a disk-like structure, with a slight elongation, but no obvious spiral arms or other distinct features are immediately apparent. There are hints of a central concentration of light, potentially a bulge. Given its moderate redshift and size, this galaxy is quite luminous. There seems to be minor disturbances present in the galaxy. No other galaxies are nearby that it seems to be merging with. 
