The galaxy presents as a relatively compact, centrally concentrated object. The morphology appears primarily smooth, with little indication of spiral arms or significant disk structures. The light distribution indicates a slight elongation, not quite circular but not highly elongated either. The core region exhibits a bright, possibly active galactic nucleus. There's a subtle color gradient visible, transitioning from a redder hue in the central region to a bluer hue in the outer regions of the galaxy, potentially indicative of differing stellar populations or dust distribution. There may be minor disturbances or interactions, as the outer edges are slightly irregular, though a more definitive observation would be needed.
