The galaxy presents as a moderately inclined, late-type spiral system. Its color index suggests ongoing star formation, particularly noticeable in the bluer regions throughout the disk. Faint, patchy spiral arms are visible, lacking grand design structure, indicating a flocculent arm morphology. The central bulge is not prominent; the luminosity distribution within the galaxy shows a disk-dominated profile with no strong central concentration. There is evidence of minor disturbances in the galaxy's morphology; potentially from past interactions. The system is considered to be a fairly average mass galaxy with a relatively normal rate of star formation for its size.
