The galaxy presents as an elongated, cigar-shaped structure. Its overall appearance suggests a relatively smooth morphology, with a concentrated central bulge. The light distribution is somewhat uniform, showing a slight fading from the center to the edges. A blueish tint is visible, possibly indicating the presence of younger stars or active star-forming regions, although at a seemingly low rate based on the smooth structure. There are no apparent signs of major disturbances or ongoing mergers, although a slight asymmetry cannot be ruled out. The galaxy's intermediate roundness implies it is viewed at a significant angle relative to its plane.
