The galaxy presents a spiral morphology, exhibiting well-defined spiral arms. A central bulge is visible, appearing of moderate size relative to the galactic disk. The spiral arms appear to be tightly wound. There may be two dominant spiral arms, with hints of additional structure. The galaxy is viewed at an angle oblique to its plane of symmetry. The color distribution suggests a central concentration of older stars, with bluer hues evident in the spiral arms, indicative of ongoing star formation. A slight asymmetry in the distribution of light may suggest a minor gravitational interaction.
