The galaxy exhibits a flattened, disk-like morphology, presenting itself nearly edge-on from our line of sight. A central bulge is present, appearing as a concentrated region of light with a yellowish-orange hue, suggesting a population of older stars. The disk component appears bluish, indicative of younger stars and potential ongoing star formation. Dust lanes are suspected along the galactic plane, although the resolution limits a clear identification. The galaxy's overall shape indicates a system dominated by rotational dynamics, consistent with a spiral or lenticular galaxy classification. The outer regions of the disk fade gradually, suggesting the presence of a stellar halo. No obvious signs of tidal disturbances or major mergers are apparent, however there seems to be a minor disturbance.
