The galaxy presents as a spiral galaxy, displaying a notable disk structure. The central bulge region exhibits a concentrated luminosity, suggesting a relatively high stellar density. Spiral arms are clearly visible, extending outwards from the central bulge. The arms appear tightly wound and demonstrate a fragmented morphology, potentially indicative of ongoing star formation regions or dust lane obscuration. Overall, the light distribution implies that the structure is not perfectly face-on; it is somewhat inclined. The galaxy does not appear to be undergoing any major merging events, though a possible minor disturbance can not be ruled out.
