The galaxy appears as a faint, elongated structure. Its morphology suggests it is likely an elliptical or lenticular galaxy, exhibiting a smooth, diffuse light distribution. The galaxy is elongated, with a notable cigar shape. No spiral arms or distinct features are visible. There may be a slight central condensation, though the resolution limits definitive identification of a prominent nucleus. The color appears relatively uniform across the galaxy, without noticeable variations in stellar population. There is no indication of active star formation regions or significant dust lanes from what is visible in this image. Based on the smooth appearance and shape, it is unlikely to be undergoing any major merger events, though the elongated structure could suggest a minor interaction in its past.
