The galaxy presents a generally smooth morphology, with a primarily elliptical shape. There is no obvious disk structure or spiral arm features present, with a fairly uniform brightness distribution. The galaxy appears to be dominated by older stellar populations, indicated by the redder color in the galaxy's core and outer regions with a distinct greenish tint. The central region exhibits a higher surface brightness, suggesting a concentration of stars towards the galactic nucleus. There is no strong evidence of recent major merger activity, although a subtle asymmetry or faint tidal feature cannot be completely ruled out without further analysis. Overall, the galaxy appears to be a fairly relaxed, evolved system.
