The observed galaxy presents a disk-like morphology. It appears inclined relative to our line of sight. The central region exhibits a concentrated, bright bulge that gradually fades into a more diffuse disk. Within the disk, spiral arm structures are discernible, appearing tightly wound around the central bulge. A bar structure is suspected due to increased density near the bulge. The spiral arms display a patchy distribution of light, suggesting regions of active star formation. The bluer colors are likely due to the presence of younger stars. The galaxy does not show obvious signs of recent major merger activity but minor disturbances may be occurring.
