The galaxy appears to be a spiral galaxy, viewed nearly edge-on. A prominent disk structure is visible, with the dust lane obscuring a portion of the galactic bulge. The bulge itself exhibits a spheroidal morphology. There is no clear indication of a strong bar structure, but a faint disturbance can be seen on the periphery. The color gradient suggests active star formation. The galaxy appears relatively isolated, with no obvious signs of major mergers or strong tidal interactions with nearby galaxies.
