This galaxy appears to be an elliptical galaxy, displaying a smooth, relatively featureless morphology. The light is concentrated in a central bulge, which emits light in the yellow wavelengths, suggesting a population of older stars. The galaxy is generally round. There is no obvious spiral arm structure or dust lanes visible in this image. The outer regions of the galaxy gradually fade into the background, indicating a lack of recent or significant star formation activity. The galaxy's classification would suggest a low star formation rate. No signs of tidal disruption or merger activity are present.
