The observed galaxy presents as a disk galaxy, viewed at a relatively high inclination, appearing close to edge-on. There is a slight warp visible in the disk. The galaxy exhibits a distinct disk structure with evident spiral arm features, though they appear somewhat flocculent rather than grand design.

There appears to be a small central bulge, although the light concentration is not particularly high, suggesting a less prominent bulge component. The disk exhibits a somewhat clumpy appearance, possibly indicating ongoing star formation regions. The presence of these star forming regions is further supported by the bluer hue in portions of the disk.
