The galaxy presents as a relatively smooth and rounded structure. There is a slight elongation in the morphology but it is very round overall. Based on the single image, the galaxy appears to lack prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. No signs of major mergers or significant tidal disturbances are present. The galaxy exhibits a subtle color gradient, appearing slightly bluer towards the outer regions and yellower near the center, though the gradient is faint, suggesting a relatively homogenous stellar population. Overall, the galaxy appears to be a quiescent system, undisturbed, with a large fraction of old stars, however there is still some star formation.
