The object appears to be a spiral galaxy, observed nearly edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge region and portions of the disk. The central bulge exhibits a moderate concentration of light, appearing slightly elongated and somewhat boxy. The stellar population in the bulge appears relatively old, indicated by its reddish-yellow hue.

The galactic disk displays a faint, bluish-white glow, suggesting the presence of younger stars and star-forming regions within the disk. The light distribution is noticeably attenuated in some areas due to dust absorption. No distinct spiral arm structures are readily discernible from this angle. The galaxy appears relatively isolated, showing no signs of major tidal disturbances or ongoing mergers. Overall, the galaxy exhibits a moderate level of star formation.
