The target galaxy exhibits a disturbed morphology, suggestive of ongoing interaction or recent merger activity. The primary component of the galaxy appears as a somewhat amorphous, elongated structure. Evident within this structure is a brighter, more compact core region. Extended emission is apparent from the core, particularly extending as a tidal tail. The color gradient across the galaxy indicates varying stellar populations and dust content. A second, distinct component is situated close to the main galaxy, and appears as another compact area with a blue hue. This component could represent either a second galactic core or a region of intense star formation triggered by the interaction. The overall structure lacks a clearly defined spiral or elliptical shape. There is a hint of potential extended emission or faint tidal features, suggesting gravitational disturbances.
