The galaxy appears to be a disk galaxy, oriented approximately edge-on to our line of sight. There is a bright, concentrated central bulge with a high surface brightness. The disk appears relatively smooth, with little evidence of strong spiral arm structure. The overall color of the galaxy appears to be dominated by green wavelengths, suggesting a potential population of ionized gas or recent star formation. A slight asymmetry is observed in the disk, with a faint extension on one side, potentially indicating a minor interaction or tidal disturbance.
