The galaxy presents an overall elliptical morphology, appearing largely smooth with a high degree of central concentration. Its shape deviates slightly from perfectly circular, exhibiting a moderate elongation along one axis. A color gradient is discernible, with the galactic center exhibiting redder hues indicative of an older stellar population or dust obscuration, while the outer regions show bluer tones, potentially associated with younger, hotter stars. There is a subtle indication of possible tidal disturbances.
