The galaxy appears to be a disk galaxy, viewed at a high inclination, potentially approaching edge-on. It exhibits a prominent central bulge, appearing yellow-white in color, suggesting an older stellar population. Fainter, bluer regions are visible along the disk, indicating ongoing star formation. There are slight visual asymmetries and the possible presence of faint tidal features or distortions, suggesting potential past or ongoing interactions with another galaxy. The main body appears to be smooth, with a lack of clear spiral arm structure. It possesses an estimated mass of 10^10.8 solar masses, and moderate levels of ongoing star formation.