The galaxy presents as a flattened, disk-like structure with a centrally concentrated region. Its dominant color is a pale bluish-white, indicating a population of relatively young, hot stars within the central region and disk. There is no obvious spiral arm structure, but it cannot be ruled out due to the quality of the image. The outer edges of the disk appear somewhat irregular and less defined. The disk is oriented roughly edge-on. There is some evidence of a faint, diffuse halo surrounding the disk, extending slightly beyond the main body of the galaxy. The image suggests the possibility of minor gravitational disturbance or interaction, based on the asymmetry, but it is also possible the disturbances are due to image processing artifacts. Overall, the galaxy appears to be relatively isolated.
