The galaxy presents as a spiral, characterized by a prominent central bulge surrounded by a disk. The spiral arms appear tightly wound, displaying a flocculent structure with localized star formation regions. The color distribution suggests a mix of stellar populations, with a yellowish core possibly indicating older stars within the bulge, and bluer hues evident in the spiral arms, which indicates a more prominent population of younger, massive stars. A bar is either absent or is relatively weak within the central region of the galaxy. The galaxy shows no obvious signs of significant recent merger activity, although there are some subtle disturbances that could indicate past or ongoing interactions. The light distribution indicates a moderate concentration, with the majority of the light emanating from the inner regions and a gradual fading towards the outer disk. The galaxy is mostly viewed face on with slight tilt.
