The observed galaxy presents a clear spiral structure, with loosely wound arms extending from a central bulge. The bulge appears moderately sized relative to the disk, suggesting a later-type spiral. The spiral arms are distinct and exhibit a flocculent morphology. The dust lanes throughout the galaxy, especially in the spiral arms, are very strong and may be hiding ongoing star formation. There is possible evidence of a bar-like structure bisecting the bulge, although this is uncertain due to the angle of observation. No other galaxies are seen to be nearby, but the spiral arms are showing a degree of distortion, which means it may have experienced a relatively minor merger, in the past.