The galaxy exhibits a prominent spiral structure, demonstrating two clearly defined arms emanating from the central bulge. The arms are moderately wound, displaying both areas of relatively tight curvature and regions where they become more extended. Areas within these spiral arms appear to exhibit increased levels of star formation. 

The galaxy has a notable central bulge, which appears neither overly dominant nor particularly small when compared to the overall galactic disk. The luminous bulge suggests a moderate concentration of older stellar populations within this central region. The galaxy's disk is observed at an angle, not quite edge-on nor face-on.

The galaxy does not present with strong disturbances or indications of ongoing major merger activity. However, subtle irregularities in the arm structure may suggest minor gravitational interactions. The galaxy has an estimated size of around 7 kpc. The overall light distribution suggests ongoing star formation within the disk, contributing to the observed bluer colors in the spiral arms.
