The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests it is largely composed of older stellar populations. The galaxy displays a yellowish hue, indicative of a lack of significant recent star formation and a dominance of redder, evolved stars. There is no visible spiral arm structure, suggesting that the galaxy is either an elliptical or lenticular type. The morphology suggests that it has undergone very few if any mergers in its history. The lack of blue light indicates a low specific star formation rate. The shape is mostly round, showing no significant elongation.
