The galaxy appears to be a spiral type, exhibiting a well-defined disk structure with prominent spiral arms. The arms are tightly wound and possess a flocculent morphology, with numerous regions of active star formation visible as bright, blue knots. The central bulge is moderately sized relative to the disk and displays a smooth, concentrated light profile. The disk's inclination is relatively face-on, allowing for a clear view of the spiral arm structure. There is no immediately visible evidence of a strong bar feature bisecting the bulge. Overall, the galaxy seems to be in a relatively undisturbed state, with no major signs of ongoing or recent merger activity, although minor disturbances cannot be ruled out. The color indices suggest a moderate level of star formation activity, contributing to its relatively blue appearance.
