The galaxy presents as an edge-on or highly inclined disk galaxy. There is a noticeable flattened structure with a high aspect ratio. The disk appears relatively smooth, with no obvious signs of strong spiral arm structures or prominent dust lanes. The bulge appears to be minimal or non-existent, with the light distribution appearing relatively uniform across the disk. The galaxy has a blue-ish hue, possibly indicating a significant population of young, hot stars. The overall morphology suggests a disk galaxy with little to no prominent bulge, and minimal signs of ongoing or recent major merger activity. Some slight irregularity on the edges of the disk could be indicative of minor disturbances or interactions.
