The galaxy appears to be an elliptical galaxy, characterized by a smooth and relatively featureless morphology. It has a centrally concentrated brightness profile, with a core that is relatively bright and gradually fades outwards. The galaxy exhibits an overall rounded shape, with no discernible spiral arms or disk-like structure. There is a hint of color variation within the galaxy, with the central region appearing slightly redder than the outer regions. This suggests a potential difference in stellar populations, with the core possibly containing older, redder stars. No signs of significant tidal disturbances or merging activity are readily apparent.
