The galaxy presents an elliptical morphology, appearing as a somewhat flattened spheroid. The central region exhibits a significantly higher surface brightness, suggesting a dense concentration of stars or an active galactic nucleus. The light distribution gradually decreases from the core outwards, with a smooth transition. The primary color of the galaxy is bluish white, with a slightly reddish tinge on both ends of the minor axis. The galaxy does not display any distinct spiral arms or prominent dust lanes. The light is consistent with a population of relatively young stars. There may be subtle distortions in its overall shape, suggesting a possibility of a past or ongoing gravitational interaction with another galaxy.
