The galaxy presents as an elongated, disk-like structure viewed nearly edge-on. A prominent central bulge is visible, exhibiting a rounded morphology. There's a suggestion of a darker dust lane bisecting the galaxy, particularly apparent near the central bulge. The disk shows some areas with clumpy structure and a non-uniform distribution of light, potentially indicating regions of active star formation. No major merger events are indicated, and the overall structure looks relatively undisturbed. The galaxy has a moderate luminosity and a mass typical of a large spiral galaxy. Colors suggest the presence of both older stellar populations (redder hues) and younger, bluer stars, indicative of ongoing, but not exceptionally high, star formation.
