The galaxy presents as a singular, relatively smooth object with an elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggesting a significant stellar population. The observed light distribution transitions gradually from the core outwards, with a radial falloff in brightness indicating a decreasing stellar density. There's a slight color gradient, the central region appears more yellow/orange, and the outer regions have a blue/green tinge, potentially indicative of variations in stellar populations and/or dust distribution. No distinct spiral arms or bar structures are clearly visible, which supports a classification favoring an elliptical or lenticular system. There is a hint of minor asymmetrical distortion that could be an ongoing merger.
