This galaxy appears to be a spiral galaxy, viewed nearly edge-on. A bright central bulge dominates the galaxy’s structure, exhibiting a high degree of symmetry. The disk is prominent and relatively thin, extending from the central bulge. The overall color is bluish, particularly in the disk, suggesting the presence of a younger stellar population and ongoing star formation. Dust lanes are not clearly visible, possibly due to the nearly edge-on orientation or limited image resolution. There is no obvious evidence of a strong bar structure or major merging activity. The outer regions of the disk appear smooth. The bulge appears less smooth than the disk. The galaxy exhibits no signs of tidal tails or other significant disturbances in its morphology.
