The galaxy presents as a somewhat elongated structure, exhibiting a diffuse, bluish hue indicative of active star formation. The light distribution is relatively smooth, although hints of subtle features or disturbances are present, potentially suggesting past or ongoing minor interactions or internal dynamics. The overall morphology appears to be transitioning away from a pure spiral, towards a more lenticular, or perhaps even elliptical system. Evidence points towards a system that, while not currently undergoing major mergers, is exhibiting some level of disturbance and active, but low, star formation.
