This galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. There is evidence of a slight elongation in its overall shape, deviating somewhat from a perfectly circular form. The central region exhibits a brighter, yellowish-white hue, suggesting a concentration of older stellar populations or significant dust obscuration. The outer regions display a fainter, bluish tinge which may indicate ongoing star formation. There is a slight distortion in the morphology of the galaxy, possibly due to a minor gravitational interaction or internal instabilities. It does not appear to be undergoing a major merger, although there is a hint of a possible tidal feature or disturbance in the galactic halo.
