The galaxy presents a relatively face-on orientation. The spiral structure is prominent, displaying multiple arms with a tightly wound morphology. Star formation appears active, with noticeable blue hues tracing the spiral arms, indicative of younger stellar populations. A central bulge is present, appearing moderately sized and characterized by a smoother, yellowish light, likely dominated by older stars. The overall shape is fairly circular, exhibiting a high degree of axial symmetry, suggesting a relatively undisturbed morphology. There is no obvious strong bar structure bisecting the galactic center. Indications of any major merger events or significant tidal disturbances are absent.
