The galaxy exhibits an elliptical morphology. Its central region presents a bright, concentrated core, suggesting a high stellar density. The light profile appears smooth and centrally concentrated. The galaxy is elongated with a well defined shape. The light of the galaxy exhibits a reddish hue, potentially indicative of an older stellar population, and/or the effects of redshift at its distance. There is no obvious sign of any spiral arms or dust lanes. No tidal features or distortions are apparent, and the light profile is smooth.
