The galaxy presents as a lenticular or possibly an edge-on spiral, with a distinct elongated shape. The central bulge region appears relatively smooth and concentrated, while the disk component is fainter and extends laterally. There is evidence of some blueish light concentrated in the disk, suggesting the possibility of recent or ongoing star formation. There is some minor dust or morphological disturbance. The overall color index suggests an intermediate population of stars, neither exclusively young blue stars, nor predominantly old red stars.
