The galaxy appears to be a disk galaxy, seen edge-on or at a highly inclined angle. A distinct central bulge is visible, appearing yellowish, likely indicating an older stellar population. The disk component shows a bluer hue, suggesting the presence of younger, hotter stars and ongoing star formation. The disk itself is relatively smooth, lacking prominent spiral arm structures, which hints that it is a lenticular galaxy. The galaxy exhibits an elongated shape, with a noticeable dust lane running along its major axis, obscuring light from the bulge and contributing to the reddening of the disk. Overall, the galaxy appears to be relatively evolved.
