The galaxy presents as a relatively smooth, elliptical-like structure, with a high degree of central concentration. There is little discernible disk or spiral arm structure apparent in the image. The light distribution suggests a mostly homogenous stellar population. Its color indices indicate a redder galaxy, possibly indicating an older stellar population and/or significant dust extinction. There may be a hint of faint disturbance in its overall morphology but no clear signs of ongoing mergers are visible. The galaxy is moderately luminous, indicating a sizable stellar mass.
