The galaxy presents as a centrally concentrated elliptical morphology. It appears predominantly smooth in structure, with no discernible spiral arms or bar features visible. The color profile indicates a redder hue, suggestive of an older stellar population with lower rates of ongoing star formation. There are no obvious signs of recent or ongoing mergers, and it appears relatively undisturbed in its immediate environment. The galaxy's shape is predominantly round, with minimal ellipticity. Based on its integrated light and overall appearance, this is likely a massive elliptical galaxy.
