The galaxy presents as a largely featureless, centrally concentrated object. It exhibits a smooth, elliptical morphology, with a high degree of roundness, suggestive of an early-type galaxy. The color appears to be reddish, which could be caused by the starlight from an older stellar population. Any arms or spiral structure are not immediately obvious, suggesting a generally homogenous distribution of light across the galactic body. There is no evidence of any major mergers or significant tidal disturbances in its structure. The galaxy appears undisturbed and relatively isolated.
