The galaxy presents as a moderately inclined spiral with a central bulge that appears somewhat prominent, with an average size with respect to the rest of the galaxy. The arms are faintly visible, suggesting it is likely that the spiral structure is loosely wound and not tightly packed. The galaxy appears to have a noticeable bar-like structure across its center, as evidenced by the elongated bright region spanning the galaxy's core. There's an absence of any signs of recent major merger activity, though possible minor disturbances may be present. The color gradient from the core outwards suggests ongoing star formation within the disk, particularly in the bluer regions of the spiral arms. The galaxy does not appear perfectly symmetrical.
