The galaxy presents as a somewhat irregular, flocculent spiral type, although its disk is not sharply defined, it's more diffuse. It is mostly blue in color, implying relatively recent or ongoing star formation activity, particularly in the brighter central region and surrounding regions. There's a hint of elongation, and a slight tilt relative to our line of sight. It appears to be a late-type spiral galaxy, likely a Sc or Sd type, with a moderately inclined disk. There are possible faint spiral arm structures. Some disturbances are visible suggesting a possible recent minor merger event. The galaxy appears to be relatively isolated.
