The galaxy appears as a centrally concentrated object with a relatively smooth morphology. Its shape is approximately round, showing minimal deviation from circular symmetry. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population and lower levels of active star formation. There's a subtle color gradient, with the outer regions of the galaxy appearing slightly bluer, hinting at the presence of some younger stars, though not dominating the overall light. There is no discernable spiral structure or prominent disk features visible in the image, leading to the preliminary classification as a galaxy with a smooth structure. Faint asymmetrical features are visible, suggesting the possibility of minor interactions or internal disturbances. However, there is no evidence to suggest an ongoing major merger event.
