This galaxy appears to be a spiral galaxy, viewed at a high inclination, though not quite edge-on. The central bulge appears small or negligible and is not distinctly separated from the disk. There is some evidence of a bar structure crossing the center of the galaxy, though this is not strongly defined. The spiral arms are somewhat flocculent and are not tightly wound. The color suggests the presence of both older stellar populations and ongoing star formation within the disk, with bluer regions interspersed throughout. The galaxy exhibits some irregularities suggesting a possible interaction or merger event. Notably, there is a slight distortion in the overall shape, and some features seem slightly offset or disturbed. Some faint dust lanes are possibly visible. The size is relatively small.