The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a noticeable reddish hue, possibly indicating a concentration of older stellar populations or dust obscuration. The outer regions display a somewhat smoother, more diffuse appearance, fading into the background. The galaxy's overall structure appears relatively undisturbed, though the data indicate the possibility of only minor disturbances. The galaxy appears to be relatively smooth without the presence of spiral arms.
