The galaxy appears as a relatively smooth, centrally concentrated object. Its color profile transitions from a yellowish core to a more greenish outer region, potentially indicating variations in stellar populations or dust content. The morphology suggests a high degree of central symmetry, with a generally rounded appearance. There might be some minor disturbances in the outer edges of the galaxy. At this resolution, no distinct spiral arms or bar structures are discernible. The galaxy exhibits a certain level of star formation.
