The galaxy presents as a lenticular or possibly an edge-on spiral system at a redshift of approximately 0.15. It exhibits a central bulge that appears yellowish-white, suggesting an older stellar population. Surrounding the bulge is a disk structure that appears bluish-white, indicating the presence of younger, hotter stars. The galaxy's overall morphology is somewhat elongated, with a cigar-like shape. There is no obvious indication of ongoing major mergers or significant tidal disturbances, although a slight asymmetry in the outer regions might suggest minor interactions or internal processes. The smoothness of the light distribution dominates, with a significant fraction of its light concentrated in a relatively smooth profile.
