The galaxy presents as a relatively smooth object with a central bulge that is slightly elongated. The light distribution is dominated by a bright, concentrated core, exhibiting a bluish hue. The blue color suggests the presence of a younger stellar population with ongoing star formation. Fainter, less structured extensions appear around the primary body of the galaxy. The smoothness of the galaxy indicates that it may be an early-type spiral galaxy, like an Sa or Sb galaxy. There might be signs of minor disturbance but further observations and analysis are needed to confirm.
