The galaxy presents as an edge-on disk galaxy. The central bulge appears prominent and elongated, exhibiting a yellowish-orange hue suggesting an older stellar population. The disk is visible extending outwards from the bulge, with hints of bluer regions concentrated along the edges. The dust lane obscuring parts of the disk is not as prominent as the bulge. The smooth appearance and high fraction of edge-on disks indicate that the galaxy is stable and not currently undergoing any major mergers or significant disturbances. Star formation is occurring at a moderate rate within this galaxy.
