The galaxy presents as an edge-on spiral, exhibiting a high degree of inclination relative to the observer's line of sight. A prominent central bulge is visible, displaying a smooth, rounded morphology and appearing yellowish in color, indicative of an older stellar population. The disk is elongated and appears relatively thin, extending outwards from the bulge. There is a hint of a faint dust lane bisecting the disk along the mid-plane, obscuring the light from stars behind it. The disk appears somewhat patchy with some areas brighter and redder than others. Based on its morphology, the galaxy is undergoing limited star formation and is not experiencing any significant mergers or interactions with other galaxies, with a mass likely greater than 10^11 solar masses. The galaxy does not present strong spiral arm features.
