The galaxy presents as a spiral galaxy with a noticeable central bulge. The spiral arms appear to be loosely wound and extended, displaying a somewhat flocculent structure. The bulge region exhibits a yellowish hue, potentially indicating an older stellar population within. The disk of the galaxy shows a bluer color, suggestive of ongoing star formation and the presence of younger, hotter stars. The galaxy is moderately inclined relative to our line of sight, allowing for a partial view of its spiral structure. The overall morphology suggests a galaxy that has not experienced major mergers recently, although some minor disturbances may be present in the outer disk.
