The galaxy presents as a relatively smooth, disk-shaped object with a noticeable bulge. The disk appears to be oriented edge-on or nearly edge-on from our line of sight. The central region exhibits a reddish hue, possibly indicating an older stellar population or significant dust obscuration. Moving outward from the center along the plane of the disk, the color shifts towards green, potentially suggesting the presence of younger, hotter stars and ongoing star formation activity. The outer edges of the disk appear somewhat diffuse and indistinct, making it difficult to precisely determine the galaxy's full extent. There is no obvious evidence of strong tidal interactions or major mergers in the form of prominent tails or distorted features. The overall appearance suggests a spiral or lenticular galaxy undergoing moderate levels of star formation.
