The galaxy presents as a spiral type, exhibiting well-defined spiral arms extending from a central bulge. The spiral arms appear grand design with an intermediate winding, showing moderate pitch angles. The galaxy presents with a distinct, moderately sized bulge that contributes significantly to the overall luminosity of the galaxy. The galactic disk appears somewhat inclined relative to our line of sight, but is clearly disk-shaped. The galaxy is well-defined and isolated with no obvious signs of recent merger events, but there are some hints of minor disturbance in the disk. Evidence of active star formation exists throughout the spiral arms of the galaxy. These regions are readily identified through their color contrast. There is evidence of a central bar-like structure.
