The galaxy presents a spiral structure, with a relatively bright, moderately sized bulge. It appears the galaxy is tilted at an angle with respect to our line of sight. Faint spiral arms are observed extending from the central bulge. The winding of these spiral arms appears of medium tightness. The arms contain some bluer regions, suggestive of ongoing star formation. The overall color of the galaxy suggests a mix of stellar populations, with bluer arms and a yellower bulge. Some minor disturbances may be present in the disk, suggestive of possible past or ongoing interactions.
