The galaxy presents as a relatively smooth, lenticular or early-type spiral structure. It exhibits a moderately bright, concentrated central bulge. A faint, flattened disk component surrounds the bulge, and seems to fade in intensity with distance from the galactic center. The disk appears nearly edge-on, with a slight inclination visible. There is little evidence of strong spiral arm structures within the disk. The galaxy is yellowish-white in color, suggesting an older stellar population. No significant dust lanes or prominent star-forming regions are clearly visible, implying a low star formation rate. There is no obvious signs of tidal disturbances or interactions with neighboring galaxies. The galaxy has an elongated, but rounded shape.
