The object appears to be a spiral galaxy viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. The disk component is elongated and appears relatively smooth, lacking significant visible dust lanes or distinct spiral arm structures. The absence of blue regions indicates low levels of current star formation activity. Overall, the galaxy presents a lenticular morphology, transitioning from a typical spiral to an elliptical shape, which is commonly associated with intermediate galaxies.
