The galaxy presents a disturbed morphology, possibly indicative of a merger event. There are no distinct spiral arm structures visible. One portion of the object exhibits a smooth, somewhat elliptical profile with a reddish hue. Adjacent to this is a more amorphous, blue-tinted region. This could be a secondary component involved in the interaction, or an area of enhanced star formation triggered by the merger. The overall appearance suggests an ongoing or recent gravitational interaction disrupting the galaxy's original structure.
