The galaxy presents as an edge-on spiral or lenticular galaxy. It appears to have a distinct central bulge that is elongated along the major axis and exhibits a smooth, rounded morphology. The bulge displays a yellowish-orange hue, possibly indicative of an older stellar population. Faint extensions on either side of the bulge suggest a relatively thin disk structure. Although no distinct spiral arm features are discernible in this image, there is a slight hint of bluer areas on either side of the disk, which might indicate some ongoing star formation, however it is low. The overall smoothness of the galaxy suggests a considerable age, potentially having undergone significant disk settling. There is no clear evidence of a major merger event or tidal disturbances, but it could be undergoing a minor disturbance.
