The galaxy presents as a largely smooth, elliptical-like structure, with a concentrated central bulge. The light profile appears to be generally consistent across the major and minor axes, with some subtle elongation. There may be a hint of a very faint, diffuse disk component, but its contribution to the overall luminosity is minimal. The color is fairly consistent throughout the galaxy. The presence of any spiral arms or strong tidal features are not clearly defined, and there is no evidence of on-going mergers or any significant disturbance of its overall structure. 
