The galaxy presents as a disk galaxy observed at an edge-on or highly inclined orientation. A prominent central bulge is visible, exhibiting a yellow-orange hue, suggesting an older stellar population. Dust lanes appear present, although not sharply defined, obscuring portions of the disk. The disk itself is elongated vertically with a less defined edge, exhibiting a mottled texture, likely due to the presence of star-forming regions and dust clouds. There appears to be a slight asymmetry in the disk's overall structure, potentially indicating a gravitational interaction or minor merger event in its past. The light distribution suggests the presence of a substantial stellar mass. The galaxy shows no indications of being a spiral, likely because of the edge-on view of this galaxy.
