The object appears to be a relatively small, disk-shaped galaxy, viewed nearly edge-on. The central bulge is bright and concentrated, exhibiting a roughly symmetrical, elliptical morphology. Moving outward from the bulge, the disk becomes fainter and appears relatively smooth. The disk shows a slight bluish hue, potentially indicating the presence of younger stars. There is no discernible spiral arm structure, and the overall morphology suggests that it is likely a lenticular or early-type spiral galaxy. There is some suggestion of minor disturbances in the disk, potentially indicating a possible past interaction or merger event, but more data is necessary to confirm.
