The galaxy presents as a disc galaxy, viewed at an inclined angle. There is evidence of a central bulge that dominates the luminosity of the galaxy. The bulge appears smooth, with a high concentration of light, suggesting an older stellar population. The galactic disc is less prominent, with a fainter and more diffuse light distribution. The blue color indicates presence of some star formation activity. The galaxy does not appear to have tightly wound spiral arms. Overall, the galaxy displays features intermediate between a pure elliptical galaxy and a spiral galaxy. There is no major morphological distortion that would indicate a recent major merger event, but there are some indications of minor disturbances in the disc. The overall structure suggests that this is a relatively evolved galaxy.
