The galaxy presents as a generally smooth, elongated structure with a relatively concentrated central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. Fainter, diffuse blue light surrounds the bulge, indicating the presence of a younger stellar population and regions of potential ongoing star formation. The galaxy's shape is cigar-like, suggesting a possible elliptical morphology, though the disk may be present, just seen at an angle. There is no noticeable spiral arm structure or bar, however, the overall morphology suggests a disk galaxy seen edge-on or an elliptical galaxy. There appear to be no signs of major ongoing mergers or significant tidal disturbances. The galaxy shows no irregular morphology suggesting it is a relaxed system.
