The galaxy appears to be a relatively small, faint object. It shows a disk-like structure. The presence of a disk is somewhat obscured but can be determined by the slight elongation in one direction. The lack of defined spiral arms and the somewhat diffuse light suggest a likely late-type spiral or a lenticular galaxy seen at a high inclination. There are no signs of a central bulge. Additionally, the lack of color variation within the galaxy itself indicates a relatively uniform stellar population. There may be some minor disturbances in the shape.
