The galaxy presents as a diffuse object with a relatively small apparent size. It exhibits a disk-like morphology, although it is not sharply defined. There is a suggestion of spiral arm structure but they are not well-resolved. The galaxy's overall color profile appears reddish, potentially indicating an older stellar population or significant dust obscuration. There may be a faint tidal tail emanating from one side, indicative of a possible past gravitational interaction with another galaxy. The central region is somewhat brighter, hinting at a possible galactic bulge. There is evidence of some blue star forming regions. Given the color gradients, it is likely the galaxy has undergone some form of disturbance.
