The galaxy presents as an extended object with a moderately bright core. The overall form appears disk-like when considering the ellipticity of the isophotes. The colour profile seems relatively uniform across the galaxy, with a slight bluer tinge in the central region transitioning toward a slightly redder hue in the outer regions. This potentially suggests on going, but weak, star formation in the nuclear region. There also seems to be disturbance in the outer regions on either side of the disk, potentially indicating a minor disturbance to the structure of the galaxy.
