The galaxy presents as a complex system, potentially undergoing a merger or interaction. There is evidence of a primary, relatively smooth component that exhibits a slightly elliptical morphology. Adjacent to this, a more diffuse, disturbed structure is visible, displaying a bluer color index. A faint tidal tail or bridge-like feature appears to connect, or at least align, these two components. It's difficult to resolve individual star-forming regions but there is a degree of asymmetry and visual perturbation that suggests a departure from a relaxed, equilibrium state. The presence of both a smoother and more diffuse element indicates a possible mixture of stellar populations, with the bluer regions likely representing areas of more recent star formation. The relatively compact size suggests it is at an intermediate distance. Overall, this galaxy exhibits signs of ongoing or recent interaction that is significantly influencing its morphology and stellar content.
