This galaxy presents as a spiral type, observed at a slight angle relative to face-on. The spiral arms are well-defined, exhibiting a medium winding pattern. Two dominant arms are readily apparent. The central bulge is of moderate size relative to the disk. The overall color of the disk is bluish, indicative of recent or ongoing star formation. There is no strong evidence of a bar structure, and the bulge appears relatively smooth. The galaxy does not show any obvious signs of major mergers, though subtle disturbances cannot be ruled out.
