The galaxy presents a distinct spiral morphology. Two well-defined spiral arms are prominent, exhibiting a winding pattern of medium pitch. The arms appear continuous and traceable throughout a significant portion of the galactic disk. A central bulge of moderate size is visible. The galaxy appears to be experiencing a minor disturbance, possibly indicating a past or ongoing interaction with a smaller companion. The galaxy's overall color suggests the presence of both young and old stellar populations. There is no apparent strong bar structure.
