The galaxy presents an overall elliptical morphology, elongated along a discernible major axis. Its central region exhibits a concentrated, bright yellowish core, suggestive of an older stellar population. The luminosity appears to diminish gradually from the core outwards, showing a smooth transition to the fainter outer regions. Hints of a disk structure are present, though it is not very prominent. There is a subtle bluer component in one area of the galaxy that may hint at star formation. Overall it appears to be a massive galaxy with a moderate rate of star formation. No obvious signs of major disturbances from galactic mergers are apparent, though subtle disturbances cannot be ruled out. 
