The galaxy exhibits a predominantly smooth morphology, suggesting an elliptical or lenticular classification. It presents a centrally concentrated luminosity profile, with a gradual decrease in surface brightness extending outwards. The galaxy has a slight elongation, deviating from a perfectly circular shape. There's a subtle color gradient visible, transitioning from a more yellowish hue in the central region to slightly redder tones in the outer regions. This color distribution could indicate an older stellar population dominating the core, with potentially younger stars or dust present in the outer regions. Evidence for spiral arms or distinct features are absent in this image. There is no visual indication of active galactic nucleus activity, such as a bright central point source or prominent jets.
