The galaxy presents as a well-defined, elongated disk seen edge-on. It exhibits a prominent central bulge, which appears smooth and centrally concentrated. The bulge has a rounded shape. The disk appears relatively thin and shows little evidence of spiral arm structure or distinct features. There is a slight asymmetry, though whether it is from some disturbance or simply dust is unclear. The colour gradient suggests an older stellar population dominates the bulge, and the disk has an apparent mix of younger and older stellar populations with some dust obscuration. There are no obvious signs of a recent major merger. Overall, the galaxy appears to be a relatively quiescent, moderately massive system with ongoing star formation.
