This galaxy presents as an elongated, disk-shaped structure, viewed at a near edge-on orientation. There is a concentration of blue light towards the center, suggesting the presence of a bulge region with active star formation, or a higher density of younger, hotter stars. The disk itself appears somewhat irregular, with hints of spiral arm structures that are partially obscured by the viewing angle. There are some hints of disruption along the disk, indicating that it may have a merging component or minor disturbance. There appears to be some dust extinction occuring.
