The galaxy presents as a spiral type, with a prominent, moderately sized central bulge. The spiral arms are distinctly visible, appearing grand design with two dominant arms extending from the central bulge. The winding of these arms is intermediate; they are neither tightly wound nor very loosely defined. The arms exhibit a noticeable presence of star forming regions, indicated by the slightly bluer, more granular texture. The galaxy's disk is oriented at a slight angle to our line of sight. There is no obvious sign of a strong central bar feature crossing the bulge. No obvious signs of major disturbances are seen but the overall asymmetry suggests a possible minor interaction.
