The galaxy presents a distinct spiral structure. Two well-defined spiral arms are apparent, loosely wound around a central bulge. The bulge appears moderately sized, with a yellowish hue, suggesting an older stellar population. The spiral arms exhibit a bluer color, indicative of ongoing star formation. There's a potential bar-like structure bisecting the central bulge. The disk is not perfectly edge-on, offering a partial view of the spiral structure. There is a slight asymmetry and some noticeable disturbance in the overall shape, indicating possible recent interactions or mergers. There is a notable central concentration.
