The galaxy presents as an elongated, disk-shaped structure. Its orientation is nearly edge-on relative to our line of sight, as the disk appears highly flattened. The central region exhibits a bright, concentrated bulge that appears yellowish in color, possibly indicative of an older stellar population. Moving outward from the bulge, the disk displays a more diffuse light, showing a slight gradient, fading in brightness towards the edges of the galaxy. There are hints of possible dust lanes along the galactic plane, slightly obscuring the light from stars behind them, giving a feathered quality to the galaxy. The overall color of the disk shifts from yellow near the bulge to slightly bluer hues at the extreme edges of the galaxy, suggestive of ongoing, though low, star formation. The galaxy's disk appears relatively undisturbed, with no major signs of tidal interactions or recent merger events. The morphology suggests a spiral galaxy, possibly of type Sb or Sc, viewed nearly edge-on.
