The galaxy exhibits a flattened ellipsoidal morphology. The central bulge appears prominent and concentrated, with a relatively smooth luminosity profile. The color is generally redder, with the central region trending towards yellow, potentially indicating an older stellar population. There may be a faint disk component, but this is subtle. There are no obvious spiral arm structures or dust lanes visible in this image. The overall appearance suggests a relatively evolved galaxy with ongoing or recently ceased star formation.
