The galaxy presents as an edge-on spiral or lenticular type. A prominent central bulge is visible, exhibiting a smooth, rounded morphology with a yellowish hue, indicating an older stellar population. The disk appears elongated and relatively thin, with a noticeable dust lane obscuring portions of the light. A slight blue tinge can be observed along the edges of the disk, potentially indicating regions of more recent star formation. There is some evidence of minor disturbance or asymmetry in the disk, possibly due to a past interaction or merger. The overall appearance suggests a quiescent or slowly star-forming system.
