The galaxy presents as a somewhat elongated structure, displaying a relatively smooth appearance with a high degree of central concentration. There is a hint of a disk-like structure, though its features are not sharply defined. The overall color is slightly bluer, particularly towards the less concentrated regions. This blueish hue may suggest the presence of younger stellar populations and ongoing star formation within those areas. The galaxy appears to be relatively isolated, with no immediately apparent major signs of interaction or ongoing merger activity. It displays a notable cigar shape.
