This galaxy presents a morphology indicative of an ongoing or recent interaction or merger event. The primary component appears relatively smooth and rounded, with a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. A secondary component, located to the west of the primary body, displays a more diffuse and irregular shape with a bluer color, consistent with ongoing star formation. This suggests that the interaction may have triggered star formation within this region. The overall structure implies possible tidal features are present between the primary and secondary body, further supporting the interaction hypothesis. There also appears to be a smaller, faint companion possibly being gravitationally disrupted by the larger galaxy.
