The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. A bright central region is evident, possibly indicating a high density of stars or an active galactic nucleus. The overall color profile appears relatively uniform, trending towards warmer hues such as red and yellow, with subtle gradients towards cooler blues at the outermost edges. No distinct spiral arms or prominent dust lanes are visible. The morphology suggests a galaxy dominated by an older stellar population. The absence of clear tidal features or distortions suggests it is not currently undergoing a major merger event. The galaxy seems relatively isolated, with no immediately apparent companion galaxies or significant interaction signs.
