The galaxy presents as an elongated, cigar-shaped structure, likely a disk galaxy viewed at a high inclination. A central bulge is visible, appearing bright and yellowish, suggesting an older stellar population concentrated in the galactic nucleus. Extending outward from the bulge are faint, bluish regions that trace the spiral arms of the galaxy. These arms show evidence of ongoing star formation, indicated by their blue color. Dust lanes are subtly interspersed within the arms, particularly on the periphery, obscuring some of the starlight. There is little evidence of major mergers or significant tidal disturbances in the galaxy's morphology. The galaxy appears relatively smooth and undisturbed, with no prominent asymmetries or irregular features, potentially indicating a relatively stable and mature system.
