The galaxy presents as an edge-on disk galaxy with a prominent, centrally located bulge. The bulge appears smooth and somewhat rounded. The galactic disk is elongated and exhibits a flattened morphology, consistent with a high inclination relative to the observer's line of sight. The disk displays a subtle blueish hue, hinting at potential star forming regions, although their distribution is difficult to discern at this resolution. There are no obvious signs of strong tidal interactions or major mergers, although there is some potential sign of minor disturbances. No distinct spiral arm structures are clearly visible. Dust lanes are not readily apparent, but the concentration of light towards the galactic mid-plane suggests a disk-like distribution of interstellar material. The galaxy's overall luminosity appears moderate, placing it within the range of typical spiral galaxies at a similar distance.
