The galaxy presents as a flattened, elongated disk structure, viewed nearly edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring the central regions. The bulge component appears relatively large and exhibits a somewhat boxy shape.  The stellar population appears to be generally older and redder, with only subtle hints of bluer, younger stars clustered in certain regions of the disk.  There is no obvious sign of strong tidal interactions or recent major mergers, although there appears to be minor disturbances in its disk. No spiral arms can be clearly distinguished due to the edge-on perspective. The galaxy displays a smooth overall profile, suggesting a relatively evolved system.
