The galaxy presents as a spiral type, viewed at an oblique angle. The disk component is prominent, displaying a flocculent structure indicative of spiral arm segments. Color gradients suggest potential stellar populations, with bluer regions possibly indicating younger stars within active star-forming areas. The galaxy exhibits an overall moderate central bulge that has an orange hue, indicative of older stars. Indications of tidal features or ongoing interactions are apparent in its morphology; signs of a possible merger can be seen. No dust lanes or complex morphological features are immediately obvious, but they could be present at higher resolutions.
