The galaxy presents as a barred spiral type, exhibiting a prominent central bulge with a relatively elongated shape. The bulge appears moderately bright and smoothly textured. Spiral arms emerge from the ends of a bar structure, these arms are somewhat loosely wound and have a flocculent appearance. There appears to be an uneven distribution of star forming regions within the spiral arms and the central bulge. The disk component of the galaxy displays a noticeable inclination relative to our line of sight. Dust lanes appear patchy, indicating the presence of interstellar material. Overall, the galaxy has a moderate level of detail visible, suggesting a relatively nearby object.
