The galaxy presents as a relatively small, disk-shaped system, estimated to be roughly 5 kpc in radius. The morphology suggests a galaxy undergoing significant interaction or possibly a merger event. A notable tidal feature or distortion is visible, indicating gravitational disturbance. The central region exhibits a brighter, more concentrated area, possibly indicative of a galactic bulge or active galactic nucleus. The color profile suggests ongoing star formation, with bluer regions indicating younger stellar populations. Evidence of dust lanes is subtle but potentially present. The galaxy's overall structure appears disturbed, which aligns with the likelihood of a major merger.
