The galaxy presents as a disk-dominated system, viewed at a steep angle, approaching edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, indicative of an older stellar population. The disk component appears relatively smooth, showing a faint blueish color which may suggest lower-level star formation. There are areas of more prominent star formation within the disk component of the galaxy. No distinct spiral arm structure can be discerned in the image. Based on the lack of obvious tidal features or major distortions in morphology, the galaxy appears relatively undisturbed, with no ongoing major merging events. The overall shape leans towards an elongated form, but not dramatically so, resembling an oblate spheroid. There is a moderate amount of dust extinction.
