This galaxy presents as a spiral type, exhibiting prominent spiral arm structures. The arms appear tightly wound, emanating from a central bulge that constitutes a significant portion of the galaxy's overall luminosity. The bulge exhibits a yellowish hue, suggesting a population of older stars. A bar structure seems present, with a moderate strength, bisecting the bulge.

The spiral arms display a bluer color, indicative of younger stellar populations and active star formation. There seems to be a large degree of patchiness within the spiral arms, meaning they may not be very continuous, and have varying brightness along their length. There may be a sign of some interaction or disturbance as the symmetry of the galaxy is not perfect. The galaxy is not viewed perfectly face-on, but presents a moderate inclination relative to our line of sight.
