The galaxy appears to be a spiral type, viewed at a slight angle from face-on. The disk is prominent, exhibiting a bluish tint indicative of active star formation regions. The spiral arms are well-defined and tightly wound around the central bulge. A bright, concentrated central bulge is visible, although it does not dominate the overall structure. There's a suggestion of a bar feature bisecting the core, but it is not strongly pronounced. No major merging events or significant tidal disturbances are readily apparent. Overall, it presents as a well-formed spiral galaxy with moderate star formation activity.
