The galaxy appears as a lenticular or possibly an elliptical galaxy at a redshift of approximately 0.24, meaning we are observing it as it was roughly 3 billion years ago. The overall color profile suggests a dominance of older stellar populations, emitting more light in the redder wavelengths. It is elongated in shape, with a relatively smooth light distribution, indicating little ongoing major star formation or significant dust lanes obscuring the view. There may be a minor tidal disturbance, but not significant. Its overall smoothness indicates advanced stages of evolution, having largely exhausted its supply of gas for star formation. The galaxy is moderately massive, and it exhibits a low specific star formation rate.
