The galaxy exhibits a pronounced disk-like structure with distinct spiral arm morphology. The arms appear tightly wound and extend from a brighter, moderately sized central bulge. A bar-like feature appears to traverse the bulge region. The color distribution suggests ongoing star formation within the spiral arms, indicated by their bluer hue, while the central bulge presents a more yellowish-white color, potentially indicating an older stellar population. The disk appears somewhat inclined relative to the line of sight, as evidenced by its elliptical appearance. The structure of the galaxy does not show significant signs of recent major mergers or tidal disruption, but the galaxy shows signs of possible minor disturbances. Overall, the galaxy presents as a well-defined spiral with evidence of active star formation.
