The galaxy presents as a highly inclined, likely disc-shaped structure. The major axis is significantly longer than the minor axis, which corresponds to the observation that it is an edge-on disc galaxy. There appears to be a slight bulge visible in the center, though it is somewhat faint and elongated along the disc. The color gradient suggests a higher concentration of older stars in the central bulge and a bluer, younger stellar population along the disc. There is very little evidence of spiral arm structure. No prominent dust lanes are apparent, although there may be some subtle obscuration along the mid-plane. No significant merger events or tidal features can be seen.
