The galaxy presents as a disk galaxy, viewed nearly edge-on. There is evidence of a central bulge, appearing brighter and more concentrated than the rest of the disk. The disk itself shows a flattened structure. One side of the disk terminates abruptly. There is some indication of asymmetry in the outer regions of the disk, possibly indicating a minor interaction or disturbance. There is also a clear color gradient, bluer towards the outer edges and redder closer to the central bulge. The light suggests there may be on-going star formation present in the outer regions. There are noticeable irregularities in the overall shape.
