The galaxy presents as an elongated object, exhibiting a disk-like structure viewed nearly edge-on. The central region displays a bright, concentrated bulge, with a yellow-white hue suggestive of an older stellar population. Extending outwards from the bulge are fainter, bluish-tinted regions. The distinct color suggests the presence of younger, hotter stars, potentially indicating ongoing star formation within the galactic disk. There are indications of minor disturbances or irregularities in the outer regions of the disk, without evidence of major mergers. The bulge exhibits a rounded morphology. The overall appearance suggests a relatively massive galaxy with a significant disk component seen from an edge-on perspective, with signs of modest star formation activity.
