The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. There appears to be a primary, relatively smooth component, with an apparent size of approximately 4 arcseconds in diameter. This primary component displays a slightly elliptical shape, leaning towards round. A secondary component is visually distinct and directly interacts with the primary. The structure shows disturbances from what may be tidal forces or a merging interaction. The galaxy exhibits a color gradient with a greener nucleus and bluer regions, potentially suggesting different stellar populations and activity levels within its various regions. The apparent magnitude suggests that this is a distant object.
