The galaxy presents as a single, luminous object with a smooth and concentrated morphology. The central region exhibits a bright, yellowish hue indicative of an older stellar population. Moving outward from the core, the color subtly shifts to a redder tone, potentially indicating the presence of dust or a gradient in stellar populations. The galaxy appears slightly elongated in shape, deviating somewhat from perfect circularity. There are no immediately apparent signs of spiral arms, a bar structure, or major tidal disturbances. The overall structure suggests a relatively evolved system with a substantial spheroid component. Weak evidence exists for very minor disturbances.
