The galaxy exhibits a flattened, disk-like morphology, viewed at an inclined angle relative to our line of sight. Two prominent spiral arms emanate from a central bulge region, displaying a relatively open, loosely wound structure. Star formation appears prevalent within these arms, indicated by bluer hues and a mottled texture. The central bulge presents a smoother, more uniform appearance with yellower hues. The galaxy shows only minor asymmetries suggesting it may have experienced a minor disturbance. There is no apparent strong bar structure.
