The galaxy presents as a lenticular or spiral galaxy observed nearly edge-on from our perspective. It exhibits a prominent central bulge that appears smooth and concentrated, with a yellowish-orange hue suggesting an older stellar population. A faint, flattened disk extends outward from the bulge, though its spiral structure, if present, is difficult to resolve in the image. The disk appears relatively thin, with a color gradient transitioning from yellowish-orange near the bulge to slightly bluer tints further out. Dark dust lanes are subtly visible against the disk, particularly near the galaxy's central region, indicating the presence of interstellar medium. The overall luminosity profile suggests a relatively massive galaxy. No signs of recent major merger events or tidal disturbances are immediately apparent based on the available imagery.
