This galaxy exhibits an elongated morphology, appearing cigar-shaped. There are visible disturbances indicative of gravitational interactions, possibly including tidal features. The colour gradients suggest a mixture of stellar populations; the central regions appear yellower, potentially indicating older, redder stars, while bluer regions may point to ongoing or recent star formation. Based on the image, a merger event is a strong possibility, possibly with a secondary galactic nucleus visible. Further data would be required to assess the dynamics and history of this system more accurately.
