The galaxy presents an elongated, cigar-shaped morphology. It appears largely smooth in texture, with a concentration of light towards the center that fades outwards. A slight disk is present in the galaxy. The color gradients suggest a redder core, potentially indicating an older stellar population or dust obscuration, surrounded by bluer regions that suggest more recent star formation. The galaxy does not appear to display signs of major disturbances or ongoing merger activity, though minor gravitational interaction cannot be ruled out. There is the possibility of a companion object or tidal stream, though the resolution limits definitive confirmation.
