The galaxy presents as an edge-on spiral with a noticeable central bulge. The bulge exhibits a yellowish-orange hue, possibly indicating an older stellar population. A disk appears to extend outwards from the bulge. A dust lane bisects the galaxy along its major axis. The overall morphology shows no strong evidence of a major ongoing merger, although some minor irregularities in the disk may suggest past interactions or internal disturbances. The galaxy has an estimated stellar mass of approximately 10^10.6 solar masses and exhibits a relatively high star formation rate. The galaxy has a redshift of 0.31, which indicates that we observe this galaxy as it was when the universe was much younger.
