The galaxy appears to be a relatively smooth, elliptical galaxy. Its overall shape is elongated. The central region exhibits a bright, concentrated bulge. The galaxy displays a color gradient, appearing bluer in the outer regions, suggesting some star formation activity, although the dominant color is redder, which may be due to aging stars. There are no apparent spiral arm structures or significant dust lanes visible in the image. The morphology suggests that the galaxy is not currently undergoing any major mergers, although there may be a slight asymmetry hinting at a minor disturbance or past interaction.
