The galaxy appears to be a spiral type, displaying prominent spiral arms. The arms are somewhat loosely wound and patchy in appearance. The central bulge is moderately sized and exhibits a yellow-orange hue, suggesting an older stellar population. The spiral arms show a bluer color, indicating ongoing star formation. There is a slight asymmetry or disturbance observed in the outer regions of the disk. A possible bar structure may be present but is not clearly defined. Overall, the galaxy demonstrates a relatively smooth morphology.
