The galaxy presents a relatively smooth, elliptical morphology with a high degree of central concentration. The object appears to be a disk galaxy, seen nearly edge-on. The disk is brighter than the surrounding halo, and the galaxy appears to have undergone a relatively small amount of interactions with other galaxies in the past, if at all. There are no signs of recent or ongoing major mergers. The galaxy is slightly elongated along its major axis, but it doesn't depart drastically from a circular shape. There may be evidence of a slight disturbance in the form of a minor asymmetry in the outer regions of the disk. The galaxy appears to be relatively massive, exhibiting a high luminosity, and has an intermediate rate of star formation.
