The galaxy presents as a spiral type, observed at an oblique angle relative to its disk plane. Two prominent spiral arms emanate from the central bulge. The spiral arms are relatively loosely wound. A subtle bar structure appears to be present across the galactic nucleus. The bulge itself exhibits moderate size, exhibiting a yellowish hue indicating an older stellar population. The disk component shows a bluer color, suggestive of ongoing star formation within the spiral arms. There appears to be no significant major merger event associated with the galaxy, although a minor disturbance or interaction may be present.
