The galaxy presents an elliptical morphology, appearing mostly smooth in texture. The central bulge exhibits a bright, concentrated luminosity, suggesting a high stellar density. A faint disk or ring-like structure is potentially observed, indicated by slightly bluer colors. No clear spiral arm features are discernible. The color indices imply a stellar population with intermediate age, as evidenced by its overall color, which is redder than typical star-forming spiral galaxies. There are no apparent tidal tails or strong morphological disturbances, although there are no other galaxies nearby that could be causing disturbances. The general shape falls between perfectly round and slightly elongated.
