This galaxy presents as a classic edge-on spiral. A prominent, centralized bulge dominates the structure, exhibiting a yellowish-orange hue indicating a likely population of older, cooler stars. The disk is thin and elongated, extending outwards from the bulge, and is also a yellowish-orange color, suggesting lower rates of active star formation compared to typical blue spiral arms.

The dust lane is quite prominent, bisecting the galaxy along its major axis. It appears to be relatively uniform in width and opacity along its visible length, obscuring the light from the bulge and disk behind it. There is no obvious clumpy structure.

There is no clear evidence of any major mergers or tidal disturbances. The bulge has a rounded appearance. The features observed suggest a relatively quiescent galaxy, potentially having already transitioned beyond its peak star-forming epoch.
