The galaxy presents as a relatively luminous, disk-shaped structure seen edge-on. The central bulge is prominent, appearing bright and somewhat spheroidal, suggesting a high concentration of stars. The disk component is thin and extends outwards from the bulge, but details of spiral arm structure are not discernible at this resolution. The color appears generally reddish, possibly indicating an older stellar population or significant dust obscuration. No signs of active galactic nuclei or intense star formation regions are immediately apparent from the image. The overall morphology suggests a spiral galaxy, likely of type Sb or Sc, though the precise classification is hampered by the edge-on viewing angle. There is no sign of any merger or disturbance in its structure.