The galaxy presents as a relatively smooth, elongated structure. It exhibits a prominent central bulge that appears yellowish-white in color, suggesting an older stellar population. The disk component is less defined, showing a subtle, bluish-white hue, with no apparent distinct spiral arm structures. The overall shape is reminiscent of an elliptical or lenticular galaxy, with a significantly greater length than width. No major mergers are visible within this system, however the galaxy does show some minor disturbance. There is a suggestion of a dust lane or faint structure wrapping along the center of the galaxy.
