The galaxy presents as an edge-on spiral, exhibiting a prominent central bulge with a yellowish hue. This suggests a population of older, less massive stars within the bulge. A faint, extended disk is visible, displaying a bluer color profile indicative of ongoing star formation. Patches of slightly darker regions, possibly dust lanes, are observed within the disk, particularly along the galactic plane. The overall morphology suggests a relatively mature system that is currently forming stars at a moderate rate. There is very little indication of tidal disturbances or ongoing mergers with other galaxies.
