The galaxy presents as an elongated structure with a noticeable blue hue. It displays a relatively smooth morphology, although there is some evidence of internal structure or disturbances. One end is brighter and more concentrated, while the other end appears more diffuse. There is a possible faint tidal feature or extended plume emanating from the galaxy, further suggesting a potential interaction or past merger event. The galaxy is neither perfectly elliptical nor displaying strong spiral arm structures. It is likely a galaxy undergoing some form of morphological transformation or disturbance.
