The galaxy presents a discernible disk structure, exhibiting a predominantly face-on orientation relative to our line of sight. Evident spiral arm morphology is present, characterized by a somewhat flocculent structure. The arms show a range of color variations, with some regions displaying a bluer hue, likely indicative of recent star formation, interspersed with yellower regions, possibly indicating older stellar populations. The galactic bulge appears to be relatively small and moderately luminous compared to the overall disk brightness. A subtle disturbance in the galaxy's symmetry could be present, possibly suggesting a minor interaction or internal dynamical process. No strong bar feature is immediately apparent. The overall appearance suggests a relatively well-defined spiral galaxy, with ongoing or recent star formation activity.
