The observed galaxy presents as a highly inclined disk galaxy, viewed nearly edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge region. The bulge exhibits a concentrated brightness with a yellowish hue, suggesting an older stellar population. The disk displays a bluer color gradient moving away from the bulge, indicating ongoing star formation activity in the outer regions. The morphology is smooth with no obvious spiral arm structure. The overall appearance is consistent with a late-type spiral galaxy seen from a near-edge-on viewing angle, possibly an Sc or Sd type. There is no significant sign of any tidal disturbance or interaction with other galaxies.
