The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. A primary, relatively smooth component displays a central concentration of light. This main body appears ellipsoidal in shape and presents a yellowish-white color, indicating an older stellar population. A secondary, more diffuse component extends from the main body in a curved, tail-like structure. This "tail" is bluer in color, possibly indicating regions of ongoing star formation. The presence of this extended feature disrupts the overall symmetry of the galaxy. The outer edges of the main galaxy body display some distortion, which hints at possible tidal interactions with a smaller merging galaxy. It is also possible that the artifact fraction is the cause of these distortions and not a merger event. Some light is present between the main body and the "tail" indicating the presence of some stellar matter between the two. Overall, the light from the galaxy is relatively concentrated.