The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The light distribution is centrally concentrated with a gradual decrease in intensity towards the outer edges, giving it a diffuse appearance. The color is generally consistent across the galaxy with a slight yellowish hue, suggesting a population of older stars, this is also supported by the lack of prominent blue colors expected from younger, hotter stars in star-forming regions. There is no clear evidence of active galactic nuclei based on the images available. Based on the shape, color, and apparent smoothness, the galaxy can be preliminarily classified as an elliptical galaxy with no prominent ongoing merger events visible.
